text: # Docstrings for generated ufuncs
  #
  # The syntax is designed to look like the function add_newdoc is being
  # called from numpy.lib, but in this file add_newdoc puts the
  # docstrings in a dictionary. This dictionary is used in
  # generate_ufuncs.py to generate the docstrings for the ufuncs in
  # scipy.special at the C level when the ufuncs are created at compile
  # time.
  
  from __future__ import division, print_function, absolute_import
  
  docdict = {}
  
  
  def get(name):
      return docdict.get(name)
  
  
  def add_newdoc(place, name, doc):
      docdict['.'.join((place, name))] = doc
  
  add_newdoc("scipy.special", "sph_harm",
      r"""
      sph_harm(m, n, theta, phi)
  
      Compute spherical harmonics.
  
      .. math:: Y^m_n(\theta,\phi) = \sqrt{\frac{2n+1}{4\pi}\frac{(n-m)!}{(n+m)!}} e^{i m \theta} P^m_n(\cos(\phi))
  
      Parameters
      ----------
      m : int
         ``|m| <= n``; the order of the harmonic.
      n : int
         where `n` >= 0; the degree of the harmonic.  This is often called
         ``l`` (lower case L) in descriptions of spherical harmonics.
      theta : float
         [0, 2*pi]; the azimuthal (longitudinal) coordinate.
      phi : float
         [0, pi]; the polar (colatitudinal) coordinate.
  
      Returns
      -------
      y_mn : complex float
         The harmonic :math:`Y^m_n` sampled at `theta` and `phi`
  
      Notes
      -----
      There are different conventions for the meaning of input arguments
      `theta` and `phi`.  We take `theta` to be the azimuthal angle and
      `phi` to be the polar angle.  It is common to see the opposite
      convention - that is `theta` as the polar angle and `phi` as the
      azimuthal angle.
  
      References
      ----------
      .. [1] Digital Library of Mathematical Functions, 14.30. http://dlmf.nist.gov/14.30
      """)
  
  add_newdoc("scipy.special", "_ellip_harm",
      """
      Internal function, use `ellip_harm` instead.
      """)
  
  add_newdoc("scipy.special", "_ellip_norm",
      """
      Internal function, use `ellip_norm` instead.
      """)
  
  add_newdoc("scipy.special", "_lambertw",
      """
      Internal function, use `lambertw` instead.
      """)
  
  add_newdoc("scipy.special", "airy",
      r"""
      airy(z)
  
      Airy functions and their derivatives.
  
      Parameters
      ----------
      z : array_like
          Real or complex argument.
  
      Returns
      -------
      Ai, Aip, Bi, Bip : ndarrays
          Airy functions Ai and Bi, and their derivatives Aip and Bip.
  
      Notes
      -----
      The Airy functions Ai and Bi are two independent solutions of
  
      .. math:: y''(x) = x y(x).
  
      For real `z` in [-10, 10], the computation is carried out by calling
      the Cephes [1]_ `airy` routine, which uses power series summation
      for small `z` and rational minimax approximations for large `z`.
  
      Outside this range, the AMOS [2]_ `zairy` and `zbiry` routines are
      employed.  They are computed using power series for :math:`|z| < 1` and
      the following relations to modified Bessel functions for larger `z`
      (where :math:`t \equiv 2 z^{3/2}/3`):
  
      .. math::
  
          Ai(z) = \frac{1}{\pi \sqrt{3}} K_{1/3}(t)
  
          Ai'(z) = -\frac{z}{\pi \sqrt{3}} K_{2/3}(t)
  
          Bi(z) = \sqrt{\frac{z}{3}} \left(I_{-1/3}(t) + I_{1/3}(t) \right)
  
          Bi'(z) = \frac{z}{\sqrt{3}} \left(I_{-2/3}(t) + I_{2/3}(t)\right)
  
      See also
      --------
      airye : exponentially scaled Airy functions.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      .. [2] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/.org/amos/
      """)
  
  add_newdoc("scipy.special", "airye",
      """
      airye(z)
  
      Exponentially scaled Airy functions and their derivatives.
  
      Scaling::
  
          eAi  = Ai  * exp(2.0/3.0*z*sqrt(z))
          eAip = Aip * exp(2.0/3.0*z*sqrt(z))
          eBi  = Bi  * exp(-abs((2.0/3.0*z*sqrt(z)).real))
          eBip = Bip * exp(-abs((2.0/3.0*z*sqrt(z)).real))
  
      Parameters
      ----------
      z : array_like
          Real or complex argument.
  
      Returns
      -------
      eAi, eAip, eBi, eBip : array_like
          Airy functions Ai and Bi, and their derivatives Aip and Bip
  
      Notes
      -----
      Wrapper for the AMOS [1]_ routines `zairy` and `zbiry`.
  
      See also
      --------
      airy
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      """)
  
  add_newdoc("scipy.special", "bdtr",
      r"""
      bdtr(k, n, p)
  
      Binomial distribution cumulative distribution function.
  
      Sum of the terms 0 through `k` of the Binomial probability density.
  
      .. math::
          \mathrm{bdtr}(k, n, p) = \sum_{j=0}^k {{n}\choose{j}} p^j (1-p)^{n-j}
  
      Parameters
      ----------
      k : array_like
          Number of successes (int).
      n : array_like
          Number of events (int).
      p : array_like
          Probability of success in a single event (float).
  
      Returns
      -------
      y : ndarray
          Probability of `k` or fewer successes in `n` independent events with
          success probabilities of `p`.
  
      Notes
      -----
      The terms are not summed directly; instead the regularized incomplete beta
      function is employed, according to the formula,
  
      .. math::
          \mathrm{bdtr}(k, n, p) = I_{1 - p}(n - k, k + 1).
  
      Wrapper for the Cephes [1]_ routine `bdtr`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "bdtrc",
      r"""
      bdtrc(k, n, p)
  
      Binomial distribution survival function.
  
      Sum of the terms `k + 1` through `n` of the binomial probability density,
  
      .. math::
          \mathrm{bdtrc}(k, n, p) = \sum_{j=k+1}^n {{n}\choose{j}} p^j (1-p)^{n-j}
  
      Parameters
      ----------
      k : array_like
          Number of successes (int).
      n : array_like
          Number of events (int)
      p : array_like
          Probability of success in a single event.
  
      Returns
      -------
      y : ndarray
          Probability of `k + 1` or more successes in `n` independent events
          with success probabilities of `p`.
  
      See also
      --------
      bdtr
      betainc
  
      Notes
      -----
      The terms are not summed directly; instead the regularized incomplete beta
      function is employed, according to the formula,
  
      .. math::
          \mathrm{bdtrc}(k, n, p) = I_{p}(k + 1, n - k).
  
      Wrapper for the Cephes [1]_ routine `bdtrc`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "bdtri",
      """
      bdtri(k, n, y)
  
      Inverse function to `bdtr` with respect to `p`.
  
      Finds the event probability `p` such that the sum of the terms 0 through
      `k` of the binomial probability density is equal to the given cumulative
      probability `y`.
  
      Parameters
      ----------
      k : array_like
          Number of successes (float).
      n : array_like
          Number of events (float)
      y : array_like
          Cumulative probability (probability of `k` or fewer successes in `n`
          events).
  
      Returns
      -------
      p : ndarray
          The event probability such that `bdtr(k, n, p) = y`.
  
      See also
      --------
      bdtr
      betaincinv
  
      Notes
      -----
      The computation is carried out using the inverse beta integral function
      and the relation,::
  
          1 - p = betaincinv(n - k, k + 1, y).
  
      Wrapper for the Cephes [1]_ routine `bdtri`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "bdtrik",
      """
      bdtrik(y, n, p)
  
      Inverse function to `bdtr` with respect to `k`.
  
      Finds the number of successes `k` such that the sum of the terms 0 through
      `k` of the Binomial probability density for `n` events with probability
      `p` is equal to the given cumulative probability `y`.
  
      Parameters
      ----------
      y : array_like
          Cumulative probability (probability of `k` or fewer successes in `n`
          events).
      n : array_like
          Number of events (float).
      p : array_like
          Success probability (float).
  
      Returns
      -------
      k : ndarray
          The number of successes `k` such that `bdtr(k, n, p) = y`.
  
      See also
      --------
      bdtr
  
      Notes
      -----
      Formula 26.5.24 of [1]_ is used to reduce the binomial distribution to the
      cumulative incomplete beta distribution.
  
      Computation of `k` involves a seach for a value that produces the desired
      value of `y`.  The search relies on the monotinicity of `y` with `k`.
  
      Wrapper for the CDFLIB [2]_ Fortran routine `cdfbin`.
  
      References
      ----------
      .. [1] Milton Abramowitz and Irene A. Stegun, eds.
             Handbook of Mathematical Functions with Formulas,
             Graphs, and Mathematical Tables. New York: Dover, 1972.
      .. [2] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
  
      """)
  
  add_newdoc("scipy.special", "bdtrin",
      """
      bdtrin(k, y, p)
  
      Inverse function to `bdtr` with respect to `n`.
  
      Finds the number of events `n` such that the sum of the terms 0 through
      `k` of the Binomial probability density for events with probability `p` is
      equal to the given cumulative probability `y`.
  
      Parameters
      ----------
      k : array_like
          Number of successes (float).
      y : array_like
          Cumulative probability (probability of `k` or fewer successes in `n`
          events).
      p : array_like
          Success probability (float).
  
      Returns
      -------
      n : ndarray
          The number of events `n` such that `bdtr(k, n, p) = y`.
  
      See also
      --------
      bdtr
  
      Notes
      -----
      Formula 26.5.24 of [1]_ is used to reduce the binomial distribution to the
      cumulative incomplete beta distribution.
  
      Computation of `n` involves a seach for a value that produces the desired
      value of `y`.  The search relies on the monotinicity of `y` with `n`.
  
      Wrapper for the CDFLIB [2]_ Fortran routine `cdfbin`.
  
      References
      ----------
      .. [1] Milton Abramowitz and Irene A. Stegun, eds.
             Handbook of Mathematical Functions with Formulas,
             Graphs, and Mathematical Tables. New York: Dover, 1972.
      .. [2] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
      """)
  
  add_newdoc("scipy.special", "binom",
      """
      binom(n, k)
  
      Binomial coefficient
      """)
  
  add_newdoc("scipy.special", "btdtria",
      r"""
      btdtria(p, b, x)
  
      Inverse of `btdtr` with respect to `a`.
  
      This is the inverse of the beta cumulative distribution function, `btdtr`,
      considered as a function of `a`, returning the value of `a` for which
      `btdtr(a, b, x) = p`, or
  
      .. math::
          p = \int_0^x \frac{\Gamma(a + b)}{\Gamma(a)\Gamma(b)} t^{a-1} (1-t)^{b-1}\,dt
  
      Parameters
      ----------
      p : array_like
          Cumulative probability, in [0, 1].
      b : array_like
          Shape parameter (`b` > 0).
      x : array_like
          The quantile, in [0, 1].
  
      Returns
      -------
      a : ndarray
          The value of the shape parameter `a` such that `btdtr(a, b, x) = p`.
  
      See Also
      --------
      btdtr : Cumulative density function of the beta distribution.
      btdtri : Inverse with respect to `x`.
      btdtrib : Inverse with respect to `b`.
  
      Notes
      -----
      Wrapper for the CDFLIB [1]_ Fortran routine `cdfbet`.
  
      The cumulative distribution function `p` is computed using a routine by
      DiDinato and Morris [2]_.  Computation of `a` involves a seach for a value
      that produces the desired value of `p`.  The search relies on the
      monotinicity of `p` with `a`.
  
      References
      ----------
      .. [1] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
      .. [2] DiDinato, A. R. and Morris, A. H.,
             Algorithm 708: Significant Digit Computation of the Incomplete Beta
             Function Ratios. ACM Trans. Math. Softw. 18 (1993), 360-373.
  
      """)
  
  add_newdoc("scipy.special", "btdtrib",
      r"""
      btdtria(a, p, x)
  
      Inverse of `btdtr` with respect to `b`.
  
      This is the inverse of the beta cumulative distribution function, `btdtr`,
      considered as a function of `b`, returning the value of `b` for which
      `btdtr(a, b, x) = p`, or
  
      .. math::
          p = \int_0^x \frac{\Gamma(a + b)}{\Gamma(a)\Gamma(b)} t^{a-1} (1-t)^{b-1}\,dt
  
      Parameters
      ----------
      a : array_like
          Shape parameter (`a` > 0).
      p : array_like
          Cumulative probability, in [0, 1].
      x : array_like
          The quantile, in [0, 1].
  
      Returns
      -------
      b : ndarray
          The value of the shape parameter `b` such that `btdtr(a, b, x) = p`.
  
      See Also
      --------
      btdtr : Cumulative density function of the beta distribution.
      btdtri : Inverse with respect to `x`.
      btdtria : Inverse with respect to `a`.
  
      Notes
      -----
      Wrapper for the CDFLIB [1]_ Fortran routine `cdfbet`.
  
      The cumulative distribution function `p` is computed using a routine by
      DiDinato and Morris [2]_.  Computation of `b` involves a seach for a value
      that produces the desired value of `p`.  The search relies on the
      monotinicity of `p` with `b`.
  
      References
      ----------
      .. [1] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
      .. [2] DiDinato, A. R. and Morris, A. H.,
             Algorithm 708: Significant Digit Computation of the Incomplete Beta
             Function Ratios. ACM Trans. Math. Softw. 18 (1993), 360-373.
  
  
      """)
  
  add_newdoc("scipy.special", "bei",
      """
      bei(x)
  
      Kelvin function bei
      """)
  
  add_newdoc("scipy.special", "beip",
      """
      beip(x)
  
      Derivative of the Kelvin function `bei`
      """)
  
  add_newdoc("scipy.special", "ber",
      """
      ber(x)
  
      Kelvin function ber.
      """)
  
  add_newdoc("scipy.special", "berp",
      """
      berp(x)
  
      Derivative of the Kelvin function `ber`
      """)
  
  add_newdoc("scipy.special", "besselpoly",
      r"""
      besselpoly(a, lmb, nu)
  
      Weighted integral of a Bessel function.
  
      .. math::
  
         \int_0^1 x^\lambda J_\nu(2 a x) \, dx
  
      where :math:`J_\nu` is a Bessel function and :math:`\lambda=lmb`,
      :math:`\nu=nu`.
  
      """)
  
  add_newdoc("scipy.special", "beta",
      """
      beta(a, b)
  
      Beta function.
  
      ::
  
          beta(a, b) =  gamma(a) * gamma(b) / gamma(a+b)
      """)
  
  add_newdoc("scipy.special", "betainc",
      """
      betainc(a, b, x)
  
      Incomplete beta integral.
  
      Compute the incomplete beta integral of the arguments, evaluated
      from zero to `x`::
  
          gamma(a+b) / (gamma(a)*gamma(b)) * integral(t**(a-1) (1-t)**(b-1), t=0..x).
  
      Notes
      -----
      The incomplete beta is also sometimes defined without the terms
      in gamma, in which case the above definition is the so-called regularized
      incomplete beta. Under this definition, you can get the incomplete beta by
      multiplying the result of the scipy function by beta(a, b).
  
      """)
  
  add_newdoc("scipy.special", "betaincinv",
      """
      betaincinv(a, b, y)
  
      Inverse function to beta integral.
  
      Compute `x` such that betainc(a, b, x) = y.
      """)
  
  add_newdoc("scipy.special", "betaln",
      """
      betaln(a, b)
  
      Natural logarithm of absolute value of beta function.
  
      Computes ``ln(abs(beta(a, b)))``.
      """)
  
  add_newdoc("scipy.special", "boxcox",
      """
      boxcox(x, lmbda)
  
      Compute the Box-Cox transformation.
  
      The Box-Cox transformation is::
  
          y = (x**lmbda - 1) / lmbda  if lmbda != 0
              log(x)                  if lmbda == 0
  
      Returns `nan` if ``x < 0``.
      Returns `-inf` if ``x == 0`` and ``lmbda < 0``.
  
      Parameters
      ----------
      x : array_like
          Data to be transformed.
      lmbda : array_like
          Power parameter of the Box-Cox transform.
  
      Returns
      -------
      y : array
          Transformed data.
  
      Notes
      -----
  
      .. versionadded:: 0.14.0
  
      Examples
      --------
      >>> from scipy.special import boxcox
      >>> boxcox([1, 4, 10], 2.5)
      array([   0.        ,   12.4       ,  126.09110641])
      >>> boxcox(2, [0, 1, 2])
      array([ 0.69314718,  1.        ,  1.5       ])
      """)
  
  add_newdoc("scipy.special", "boxcox1p",
      """
      boxcox1p(x, lmbda)
  
      Compute the Box-Cox transformation of 1 + `x`.
  
      The Box-Cox transformation computed by `boxcox1p` is::
  
          y = ((1+x)**lmbda - 1) / lmbda  if lmbda != 0
              log(1+x)                    if lmbda == 0
  
      Returns `nan` if ``x < -1``.
      Returns `-inf` if ``x == -1`` and ``lmbda < 0``.
  
      Parameters
      ----------
      x : array_like
          Data to be transformed.
      lmbda : array_like
          Power parameter of the Box-Cox transform.
  
      Returns
      -------
      y : array
          Transformed data.
  
      Notes
      -----
  
      .. versionadded:: 0.14.0
  
      Examples
      --------
      >>> from scipy.special import boxcox1p
      >>> boxcox1p(1e-4, [0, 0.5, 1])
      array([  9.99950003e-05,   9.99975001e-05,   1.00000000e-04])
      >>> boxcox1p([0.01, 0.1], 0.25)
      array([ 0.00996272,  0.09645476])
      """)
  
  add_newdoc("scipy.special", "inv_boxcox",
      """
      inv_boxcox(y, lmbda)
  
      Compute the inverse of the Box-Cox transformation.
  
      Find ``x`` such that::
  
          y = (x**lmbda - 1) / lmbda  if lmbda != 0
              log(x)                  if lmbda == 0
  
      Parameters
      ----------
      y : array_like
          Data to be transformed.
      lmbda : array_like
          Power parameter of the Box-Cox transform.
  
      Returns
      -------
      x : array
          Transformed data.
  
      Notes
      -----
  
      .. versionadded:: 0.16.0
  
      Examples
      --------
      >>> from scipy.special import boxcox, inv_boxcox
      >>> y = boxcox([1, 4, 10], 2.5)
      >>> inv_boxcox(y, 2.5)
      array([1., 4., 10.])
      """)
  
  add_newdoc("scipy.special", "inv_boxcox1p",
      """
      inv_boxcox1p(y, lmbda)
  
      Compute the inverse of the Box-Cox transformation.
  
      Find ``x`` such that::
  
          y = ((1+x)**lmbda - 1) / lmbda  if lmbda != 0
              log(1+x)                    if lmbda == 0
  
      Parameters
      ----------
      y : array_like
          Data to be transformed.
      lmbda : array_like
          Power parameter of the Box-Cox transform.
  
      Returns
      -------
      x : array
          Transformed data.
  
      Notes
      -----
  
      .. versionadded:: 0.16.0
  
      Examples
      --------
      >>> from scipy.special import boxcox1p, inv_boxcox1p
      >>> y = boxcox1p([1, 4, 10], 2.5)
      >>> inv_boxcox1p(y, 2.5)
      array([1., 4., 10.])
      """)
  
  add_newdoc("scipy.special", "btdtr",
      r"""
      btdtr(a, b, x)
  
      Cumulative density function of the beta distribution.
  
      Returns the integral from zero to `x` of the beta probability density
      function,
  
      .. math::
          I = \int_0^x \frac{\Gamma(a + b)}{\Gamma(a)\Gamma(b)} t^{a-1} (1-t)^{b-1}\,dt
  
      where :math:`\Gamma` is the gamma function.
  
      Parameters
      ----------
      a : array_like
          Shape parameter (a > 0).
      b : array_like
          Shape parameter (b > 0).
      x : array_like
          Upper limit of integration, in [0, 1].
  
      Returns
      -------
      I : ndarray
          Cumulative density function of the beta distribution with parameters
          `a` and `b` at `x`.
  
      See Also
      --------
      betainc
  
      Notes
      -----
      This function is identical to the incomplete beta integral function
      `betainc`.
  
      Wrapper for the Cephes [1]_ routine `btdtr`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "btdtri",
      r"""
      btdtri(a, b, p)
  
      The `p`-th quantile of the beta distribution.
  
      This function is the inverse of the beta cumulative distribution function,
      `btdtr`, returning the value of `x` for which `btdtr(a, b, x) = p`, or
  
      .. math::
          p = \int_0^x \frac{\Gamma(a + b)}{\Gamma(a)\Gamma(b)} t^{a-1} (1-t)^{b-1}\,dt
  
      Parameters
      ----------
      a : array_like
          Shape parameter (`a` > 0).
      b : array_like
          Shape parameter (`b` > 0).
      p : array_like
          Cumulative probability, in [0, 1].
  
      Returns
      -------
      x : ndarray
          The quantile corresponding to `p`.
  
      See Also
      --------
      betaincinv
      btdtr
  
      Notes
      -----
      The value of `x` is found by interval halving or Newton iterations.
  
      Wrapper for the Cephes [1]_ routine `incbi`, which solves the equivalent
      problem of finding the inverse of the incomplete beta integral.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "cbrt",
      """
      cbrt(x)
  
      Cube root of `x`
      """)
  
  add_newdoc("scipy.special", "chdtr",
      """
      chdtr(v, x)
  
      Chi square cumulative distribution function
  
      Returns the area under the left hand tail (from 0 to `x`) of the Chi
      square probability density function with `v` degrees of freedom::
  
          1/(2**(v/2) * gamma(v/2)) * integral(t**(v/2-1) * exp(-t/2), t=0..x)
      """)
  
  add_newdoc("scipy.special", "chdtrc",
      """
      chdtrc(v, x)
  
      Chi square survival function
  
      Returns the area under the right hand tail (from `x` to
      infinity) of the Chi square probability density function with `v`
      degrees of freedom::
  
          1/(2**(v/2) * gamma(v/2)) * integral(t**(v/2-1) * exp(-t/2), t=x..inf)
      """)
  
  add_newdoc("scipy.special", "chdtri",
      """
      chdtri(v, p)
  
      Inverse to `chdtrc`
  
      Returns the argument x such that ``chdtrc(v, x) == p``.
      """)
  
  add_newdoc("scipy.special", "chdtriv",
      """
      chdtri(p, x)
  
      Inverse to `chdtr` vs `v`
  
      Returns the argument v such that ``chdtr(v, x) == p``.
      """)
  
  add_newdoc("scipy.special", "chndtr",
      """
      chndtr(x, df, nc)
  
      Non-central chi square cumulative distribution function
  
      """)
  
  add_newdoc("scipy.special", "chndtrix",
      """
      chndtrix(p, df, nc)
  
      Inverse to `chndtr` vs `x`
      """)
  
  add_newdoc("scipy.special", "chndtridf",
      """
      chndtridf(x, p, nc)
  
      Inverse to `chndtr` vs `df`
      """)
  
  add_newdoc("scipy.special", "chndtrinc",
      """
      chndtrinc(x, df, p)
  
      Inverse to `chndtr` vs `nc`
      """)
  
  add_newdoc("scipy.special", "cosdg",
      """
      cosdg(x)
  
      Cosine of the angle `x` given in degrees.
      """)
  
  add_newdoc("scipy.special", "cosm1",
      """
      cosm1(x)
  
      cos(x) - 1 for use when `x` is near zero.
      """)
  
  add_newdoc("scipy.special", "cotdg",
      """
      cotdg(x)
  
      Cotangent of the angle `x` given in degrees.
      """)
  
  add_newdoc("scipy.special", "dawsn",
      """
      dawsn(x)
  
      Dawson's integral.
  
      Computes::
  
          exp(-x**2) * integral(exp(t**2), t=0..x).
  
      See Also
      --------
      wofz, erf, erfc, erfcx, erfi
  
      References
      ----------
      .. [1] Steven G. Johnson, Faddeeva W function implementation.
         http://ab-initio.mit.edu/Faddeeva
  
      Examples
      --------
      >>> from scipy import special
      >>> import matplotlib.pyplot as plt
      >>> x = np.linspace(-15, 15, num=1000)
      >>> plt.plot(x, special.dawsn(x))
      >>> plt.xlabel('$x$')
      >>> plt.ylabel('$dawsn(x)$')
      >>> plt.show()
  
      """)
  
  add_newdoc("scipy.special", "ellipe",
      """
      ellipe(m)
  
      Complete elliptic integral of the second kind
  
      This function is defined as
  
      .. math:: E(m) = \\int_0^{\\pi/2} [1 - m \\sin(t)^2]^{1/2} dt
  
      Parameters
      ----------
      m : array_like
          Defines the parameter of the elliptic integral.
  
      Returns
      -------
      E : ndarray
          Value of the elliptic integral.
  
      Notes
      -----
      Wrapper for the Cephes [1]_ routine `ellpe`.
  
      For `m > 0` the computation uses the approximation,
  
      .. math:: E(m) \\approx P(1-m) - (1-m) \\log(1-m) Q(1-m),
  
      where :math:`P` and :math:`Q` are tenth-order polynomials.  For
      `m < 0`, the relation
  
      .. math:: E(m) = E(m/(m - 1)) \\sqrt(1-m)
  
      is used.
  
      See Also
      --------
      ellipkm1 : Complete elliptic integral of the first kind, near `m` = 1
      ellipk : Complete elliptic integral of the first kind
      ellipkinc : Incomplete elliptic integral of the first kind
      ellipeinc : Incomplete elliptic integral of the second kind
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "ellipeinc",
      """
      ellipeinc(phi, m)
  
      Incomplete elliptic integral of the second kind
  
      This function is defined as
  
      .. math:: E(\\phi, m) = \\int_0^{\\phi} [1 - m \\sin(t)^2]^{1/2} dt
  
      Parameters
      ----------
      phi : array_like
          amplitude of the elliptic integral.
  
      m : array_like
          parameter of the elliptic integral.
  
      Returns
      -------
      E : ndarray
          Value of the elliptic integral.
  
      Notes
      -----
      Wrapper for the Cephes [1]_ routine `ellie`.
  
      Computation uses arithmetic-geometric means algorithm.
  
      See Also
      --------
      ellipkm1 : Complete elliptic integral of the first kind, near `m` = 1
      ellipk : Complete elliptic integral of the first kind
      ellipkinc : Incomplete elliptic integral of the first kind
      ellipe : Complete elliptic integral of the second kind
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "ellipj",
      """
      ellipj(u, m)
  
      Jacobian elliptic functions
  
      Calculates the Jacobian elliptic functions of parameter `m` between
      0 and 1, and real argument `u`.
  
      Parameters
      ----------
      m : array_like
          Parameter.
      u : array_like
          Argument.
  
      Returns
      -------
      sn, cn, dn, ph : ndarrays
          The returned functions::
  
              sn(u|m), cn(u|m), dn(u|m)
  
          The value `ph` is such that if `u = ellipk(ph, m)`,
          then `sn(u|m) = sin(ph)` and `cn(u|m) = cos(ph)`.
  
      Notes
      -----
      Wrapper for the Cephes [1]_ routine `ellpj`.
  
      These functions are periodic, with quarter-period on the real axis
      equal to the complete elliptic integral `ellipk(m)`.
  
      Relation to incomplete elliptic integral: If `u = ellipk(phi,m)`, then
      `sn(u|m) = sin(phi)`, and `cn(u|m) = cos(phi)`.  The `phi` is called
      the amplitude of `u`.
  
      Computation is by means of the arithmetic-geometric mean algorithm,
      except when `m` is within 1e-9 of 0 or 1.  In the latter case with `m`
      close to 1, the approximation applies only for `phi < pi/2`.
  
      See also
      --------
      ellipk : Complete elliptic integral of the first kind.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "ellipkm1",
      """
      ellipkm1(p)
  
      Complete elliptic integral of the first kind around `m` = 1
  
      This function is defined as
  
      .. math:: K(p) = \\int_0^{\\pi/2} [1 - m \\sin(t)^2]^{-1/2} dt
  
      where `m = 1 - p`.
  
      Parameters
      ----------
      p : array_like
          Defines the parameter of the elliptic integral as `m = 1 - p`.
  
      Returns
      -------
      K : ndarray
          Value of the elliptic integral.
  
      Notes
      -----
      Wrapper for the Cephes [1]_ routine `ellpk`.
  
      For `p <= 1`, computation uses the approximation,
  
      .. math:: K(p) \\approx P(p) - \\log(p) Q(p),
  
      where :math:`P` and :math:`Q` are tenth-order polynomials.  The
      argument `p` is used internally rather than `m` so that the logarithmic
      singularity at `m = 1` will be shifted to the origin; this preserves
      maximum accuracy.  For `p > 1`, the identity
  
      .. math:: K(p) = K(1/p)/\\sqrt(p)
  
      is used.
  
      See Also
      --------
      ellipk : Complete elliptic integral of the first kind
      ellipkinc : Incomplete elliptic integral of the first kind
      ellipe : Complete elliptic integral of the second kind
      ellipeinc : Incomplete elliptic integral of the second kind
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "ellipkinc",
      """
      ellipkinc(phi, m)
  
      Incomplete elliptic integral of the first kind
  
      This function is defined as
  
      .. math:: K(\\phi, m) = \\int_0^{\\phi} [1 - m \\sin(t)^2]^{-1/2} dt
  
      This function is also called `F(phi, m)`.
  
      Parameters
      ----------
      phi : array_like
          amplitude of the elliptic integral
  
      m : array_like
          parameter of the elliptic integral
  
      Returns
      -------
      K : ndarray
          Value of the elliptic integral
  
      Notes
      -----
      Wrapper for the Cephes [1]_ routine `ellik`.  The computation is
      carried out using the arithmetic-geometric mean algorithm.
  
      See Also
      --------
      ellipkm1 : Complete elliptic integral of the first kind, near `m` = 1
      ellipk : Complete elliptic integral of the first kind
      ellipe : Complete elliptic integral of the second kind
      ellipeinc : Incomplete elliptic integral of the second kind
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "entr",
      r"""
      entr(x)
  
      Elementwise function for computing entropy.
  
      .. math:: \text{entr}(x) = \begin{cases} - x \log(x) & x > 0  \\ 0 & x = 0 \\ -\infty & \text{otherwise} \end{cases}
  
      Parameters
      ----------
      x : ndarray
          Input array.
  
      Returns
      -------
      res : ndarray
          The value of the elementwise entropy function at the given points `x`.
  
      See Also
      --------
      kl_div, rel_entr
  
      Notes
      -----
      This function is concave.
  
      .. versionadded:: 0.15.0
  
      """)
  
  add_newdoc("scipy.special", "erf",
      """
      erf(z)
  
      Returns the error function of complex argument.
  
      It is defined as ``2/sqrt(pi)*integral(exp(-t**2), t=0..z)``.
  
      Parameters
      ----------
      x : ndarray
          Input array.
  
      Returns
      -------
      res : ndarray
          The values of the error function at the given points `x`.
  
      See Also
      --------
      erfc, erfinv, erfcinv, wofz, erfcx, erfi
  
      Notes
      -----
      The cumulative of the unit normal distribution is given by
      ``Phi(z) = 1/2[1 + erf(z/sqrt(2))]``.
  
      References
      ----------
      .. [1] http://en.wikipedia.org/wiki/Error_function
      .. [2] Milton Abramowitz and Irene A. Stegun, eds.
          Handbook of Mathematical Functions with Formulas,
          Graphs, and Mathematical Tables. New York: Dover,
          1972. http://www.math.sfu.ca/~cbm/aands/page_297.htm
      .. [3] Steven G. Johnson, Faddeeva W function implementation.
         http://ab-initio.mit.edu/Faddeeva
  
      Examples
      --------
      >>> from scipy import special
      >>> import matplotlib.pyplot as plt
      >>> x = np.linspace(-3, 3)
      >>> plt.plot(x, special.erf(x))
      >>> plt.xlabel('$x$')
      >>> plt.ylabel('$erf(x)$')
      >>> plt.show()
  
      """)
  
  add_newdoc("scipy.special", "erfc",
      """
      erfc(x)
  
      Complementary error function, ``1 - erf(x)``.
  
      See Also
      --------
      erf, erfi, erfcx, dawsn, wofz
  
      References
      ----------
      .. [1] Steven G. Johnson, Faddeeva W function implementation.
         http://ab-initio.mit.edu/Faddeeva
  
      Examples
      --------
      >>> from scipy import special
      >>> import matplotlib.pyplot as plt
      >>> x = np.linspace(-3, 3)
      >>> plt.plot(x, special.erfc(x))
      >>> plt.xlabel('$x$')
      >>> plt.ylabel('$erfc(x)$')
      >>> plt.show()
  
      """)
  
  add_newdoc("scipy.special", "erfi",
      """
      erfi(z)
  
      Imaginary error function, ``-i erf(i z)``.
  
      See Also
      --------
      erf, erfc, erfcx, dawsn, wofz
  
      Notes
      -----
  
      .. versionadded:: 0.12.0
  
      References
      ----------
      .. [1] Steven G. Johnson, Faddeeva W function implementation.
         http://ab-initio.mit.edu/Faddeeva
  
      Examples
      --------
      >>> from scipy import special
      >>> import matplotlib.pyplot as plt
      >>> x = np.linspace(-3, 3)
      >>> plt.plot(x, special.erfi(x))
      >>> plt.xlabel('$x$')
      >>> plt.ylabel('$erfi(x)$')
      >>> plt.show()
  
      """)
  
  add_newdoc("scipy.special", "erfcx",
      """
      erfcx(x)
  
      Scaled complementary error function, ``exp(x**2) * erfc(x)``.
  
      See Also
      --------
      erf, erfc, erfi, dawsn, wofz
  
      Notes
      -----
  
      .. versionadded:: 0.12.0
  
      References
      ----------
      .. [1] Steven G. Johnson, Faddeeva W function implementation.
         http://ab-initio.mit.edu/Faddeeva
  
      Examples
      --------
      >>> from scipy import special
      >>> import matplotlib.pyplot as plt
      >>> x = np.linspace(-3, 3)
      >>> plt.plot(x, special.erfcx(x))
      >>> plt.xlabel('$x$')
      >>> plt.ylabel('$erfcx(x)$')
      >>> plt.show()
  
      """)
  
  add_newdoc("scipy.special", "eval_jacobi",
      """
      eval_jacobi(n, alpha, beta, x, out=None)
  
      Evaluate Jacobi polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_sh_jacobi",
      """
      eval_sh_jacobi(n, p, q, x, out=None)
  
      Evaluate shifted Jacobi polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_gegenbauer",
      """
      eval_gegenbauer(n, alpha, x, out=None)
  
      Evaluate Gegenbauer polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_chebyt",
      """
      eval_chebyt(n, x, out=None)
  
      Evaluate Chebyshev T polynomial at a point.
  
      This routine is numerically stable for `x` in ``[-1, 1]`` at least
      up to order ``10000``.
      """)
  
  add_newdoc("scipy.special", "eval_chebyu",
      """
      eval_chebyu(n, x, out=None)
  
      Evaluate Chebyshev U polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_chebys",
      """
      eval_chebys(n, x, out=None)
  
      Evaluate Chebyshev S polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_chebyc",
      """
      eval_chebyc(n, x, out=None)
  
      Evaluate Chebyshev C polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_sh_chebyt",
      """
      eval_sh_chebyt(n, x, out=None)
  
      Evaluate shifted Chebyshev T polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_sh_chebyu",
      """
      eval_sh_chebyu(n, x, out=None)
  
      Evaluate shifted Chebyshev U polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_legendre",
      """
      eval_legendre(n, x, out=None)
  
      Evaluate Legendre polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_sh_legendre",
      """
      eval_sh_legendre(n, x, out=None)
  
      Evaluate shifted Legendre polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_genlaguerre",
      """
      eval_genlaguerre(n, alpha, x, out=None)
  
      Evaluate generalized Laguerre polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_laguerre",
       """
      eval_laguerre(n, x, out=None)
  
      Evaluate Laguerre polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_hermite",
      """
      eval_hermite(n, x, out=None)
  
      Evaluate Hermite polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "eval_hermitenorm",
      """
      eval_hermitenorm(n, x, out=None)
  
      Evaluate normalized Hermite polynomial at a point.
      """)
  
  add_newdoc("scipy.special", "exp1",
      """
      exp1(z)
  
      Exponential integral E_1 of complex argument z
  
      ::
  
          integral(exp(-z*t)/t, t=1..inf).
      """)
  
  add_newdoc("scipy.special", "exp10",
      """
      exp10(x)
  
      10**x
      """)
  
  add_newdoc("scipy.special", "exp2",
      """
      exp2(x)
  
      2**x
      """)
  
  add_newdoc("scipy.special", "expi",
      """
      expi(x)
  
      Exponential integral Ei
  
      Defined as::
  
          integral(exp(t)/t, t=-inf..x)
  
      See `expn` for a different exponential integral.
      """)
  
  add_newdoc('scipy.special', 'expit',
      """
      expit(x)
  
      Expit ufunc for ndarrays.
  
      The expit function, also known as the logistic function, is defined as
      expit(x) = 1/(1+exp(-x)). It is the inverse of the logit function.
  
      Parameters
      ----------
      x : ndarray
          The ndarray to apply expit to element-wise.
  
      Returns
      -------
      out : ndarray
          An ndarray of the same shape as x. Its entries
          are expit of the corresponding entry of x.
  
      Notes
      -----
      As a ufunc expit takes a number of optional
      keyword arguments. For more information
      see `ufuncs <https://docs.scipy.org/doc/numpy/reference/ufuncs.html>`_
  
      .. versionadded:: 0.10.0
  
      """)
  
  add_newdoc("scipy.special", "expm1",
      """
      expm1(x)
  
      exp(x) - 1 for use when `x` is near zero.
      """)
  
  add_newdoc("scipy.special", "expn",
      """
      expn(n, x)
  
      Exponential integral E_n
  
      Returns the exponential integral for integer `n` and non-negative `x` and
      `n`::
  
          integral(exp(-x*t) / t**n, t=1..inf).
      """)
  
  add_newdoc("scipy.special", "exprel",
      r"""
      exprel(x)
  
      Relative error exponential, (exp(x)-1)/x, for use when `x` is near zero.
  
      Parameters
      ----------
      x : ndarray
          Input array.
  
      Returns
      -------
      res : ndarray
          Output array.
  
      See Also
      --------
      expm1
  
      .. versionadded:: 0.17.0
      """)
  
  add_newdoc("scipy.special", "fdtr",
      r"""
      fdtr(dfn, dfd, x)
  
      F cumulative distribution function.
  
      Returns the value of the cumulative density function of the
      F-distribution, also known as Snedecor's F-distribution or the
      Fisher-Snedecor distribution.
  
      The F-distribution with parameters :math:`d_n` and :math:`d_d` is the
      distribution of the random variable,
  
      .. math::
          X = \frac{U_n/d_n}{U_d/d_d},
  
      where :math:`U_n` and :math:`U_d` are random variables distributed
      :math:`\chi^2`, with :math:`d_n` and :math:`d_d` degrees of freedom,
      respectively.
  
      Parameters
      ----------
      dfn : array_like
          First parameter (positive float).
      dfd : array_like
          Second parameter (positive float).
      x : array_like
          Argument (nonnegative float).
  
      Returns
      -------
      y : ndarray
          The CDF of the F-distribution with parameters `dfn` and `dfd` at `x`.
  
      Notes
      -----
      The regularized incomplete beta function is used, according to the
      formula,
  
      .. math::
          F(d_n, d_d; x) = I_{xd_n/(d_d + xd_n)}(d_n/2, d_d/2).
  
      Wrapper for the Cephes [1]_ routine `fdtr`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "fdtrc",
      r"""
      fdtrc(dfn, dfd, x)
  
      F survival function.
  
      Returns the complemented F-distribution function (the integral of the
      density from `x` to infinity).
  
      Parameters
      ----------
      dfn : array_like
          First parameter (positive float).
      dfd : array_like
          Second parameter (positive float).
      x : array_like
          Argument (nonnegative float).
  
      Returns
      -------
      y : ndarray
          The complemented F-distribution function with parameters `dfn` and
          `dfd` at `x`.
  
      See also
      --------
      fdtr
  
      Notes
      -----
      The regularized incomplete beta function is used, according to the
      formula,
  
      .. math::
          F(d_n, d_d; x) = I_{d_d/(d_d + xd_n)}(d_d/2, d_n/2).
  
      Wrapper for the Cephes [1]_ routine `fdtrc`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "fdtri",
      r"""
      fdtri(dfn, dfd, p)
  
      The `p`-th quantile of the F-distribution.
  
      This function is the inverse of the F-distribution CDF, `fdtr`, returning
      the `x` such that `fdtr(dfn, dfd, x) = p`.
  
      Parameters
      ----------
      dfn : array_like
          First parameter (positive float).
      dfd : array_like
          Second parameter (positive float).
      p : array_like
          Cumulative probability, in [0, 1].
  
      Returns
      -------
      x : ndarray
          The quantile corresponding to `p`.
  
      Notes
      -----
      The computation is carried out using the relation to the inverse
      regularized beta function, :math:`I^{-1}_x(a, b)`.  Let
      :math:`z = I^{-1}_p(d_d/2, d_n/2).`  Then,
  
      .. math::
          x = \frac{d_d (1 - z)}{d_n z}.
  
      If `p` is such that :math:`x < 0.5`, the following relation is used
      instead for improved stability: let
      :math:`z' = I^{-1}_{1 - p}(d_n/2, d_d/2).` Then,
  
      .. math::
          x = \frac{d_d z'}{d_n (1 - z')}.
  
      Wrapper for the Cephes [1]_ routine `fdtri`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "fdtridfd",
      """
      fdtridfd(dfn, p, x)
  
      Inverse to `fdtr` vs dfd
  
      Finds the F density argument dfd such that ``fdtr(dfn, dfd, x) == p``.
      """)
  
  add_newdoc("scipy.special", "fdtridfn",
      """
      fdtridfn(p, dfd, x)
  
      Inverse to `fdtr` vs dfn
  
      finds the F density argument dfn such that ``fdtr(dfn, dfd, x) == p``.
      """)
  
  add_newdoc("scipy.special", "fresnel",
      """
      fresnel(z)
  
      Fresnel sin and cos integrals
  
      Defined as::
  
          ssa = integral(sin(pi/2 * t**2), t=0..z)
          csa = integral(cos(pi/2 * t**2), t=0..z)
  
      Parameters
      ----------
      z : float or complex array_like
          Argument
  
      Returns
      -------
      ssa, csa
          Fresnel sin and cos integral values
  
      """)
  
  add_newdoc("scipy.special", "gamma",
      """
      gamma(z)
  
      Gamma function.
  
      The gamma function is often referred to as the generalized
      factorial since ``z*gamma(z) = gamma(z+1)`` and ``gamma(n+1) =
      n!`` for natural number *n*.
      """)
  
  add_newdoc("scipy.special", "gammainc",
      """
      gammainc(a, x)
  
      Incomplete gamma function
  
      Defined as::
  
          1 / gamma(a) * integral(exp(-t) * t**(a-1), t=0..x)
  
      `a` must be positive and `x` must be >= 0.
      """)
  
  add_newdoc("scipy.special", "gammaincc",
      """
      gammaincc(a, x)
  
      Complemented incomplete gamma integral
  
      Defined as::
  
          1 / gamma(a) * integral(exp(-t) * t**(a-1), t=x..inf) = 1 - gammainc(a, x)
  
      `a` must be positive and `x` must be >= 0.
      """)
  
  add_newdoc("scipy.special", "gammainccinv",
      """
      gammainccinv(a, y)
  
      Inverse to `gammaincc`
  
      Returns `x` such that ``gammaincc(a, x) == y``.
      """)
  
  add_newdoc("scipy.special", "gammaincinv",
      """
      gammaincinv(a, y)
  
      Inverse to `gammainc`
  
      Returns `x` such that ``gammainc(a, x) = y``.
      """)
  
  add_newdoc("scipy.special", "_gammaln",
      """
      Internal function, use ``gammaln`` instead.
      """)
  
  add_newdoc("scipy.special", "gammasgn",
      """
      gammasgn(x)
  
      Sign of the gamma function.
  
      See Also
      --------
      gammaln
      loggamma
      """)
  
  add_newdoc("scipy.special", "gdtr",
      r"""
      gdtr(a, b, x)
  
      Gamma distribution cumulative density function.
  
      Returns the integral from zero to `x` of the gamma probability density
      function,
  
      .. math::
  
          F = \int_0^x \frac{a^b}{\Gamma(b)} t^{b-1} e^{-at}\,dt,
  
      where :math:`\Gamma` is the gamma function.
  
      Parameters
      ----------
      a : array_like
          The rate parameter of the gamma distribution, sometimes denoted
          :math:`\beta` (float).  It is also the reciprocal of the scale
          parameter :math:`\theta`.
      b : array_like
          The shape parameter of the gamma distribution, sometimes denoted
          :math:`\alpha` (float).
      x : array_like
          The quantile (upper limit of integration; float).
  
      See also
      --------
      gdtrc : 1 - CDF of the gamma distribution.
  
      Returns
      -------
      F : ndarray
          The CDF of the gamma distribution with parameters `a` and `b`
          evaluated at `x`.
  
      Notes
      -----
      The evaluation is carried out using the relation to the incomplete gamma
      integral (regularized gamma function).
  
      Wrapper for the Cephes [1]_ routine `gdtr`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "gdtrc",
      r"""
      gdtrc(a, b, x)
  
      Gamma distribution survival function.
  
      Integral from `x` to infinity of the gamma probability density function,
  
      .. math::
  
          F = \int_x^\infty \frac{a^b}{\Gamma(b)} t^{b-1} e^{-at}\,dt,
  
      where :math:`\Gamma` is the gamma function.
  
      Parameters
      ----------
      a : array_like
          The rate parameter of the gamma distribution, sometimes denoted
          :math:`\beta` (float).  It is also the reciprocal of the scale
          parameter :math:`\theta`.
      b : array_like
          The shape parameter of the gamma distribution, sometimes denoted
          :math:`\alpha` (float).
      x : array_like
          The quantile (lower limit of integration; float).
  
      Returns
      -------
      F : ndarray
          The survival function of the gamma distribution with parameters `a`
          and `b` evaluated at `x`.
  
      See Also
      --------
      gdtr, gdtri
  
      Notes
      -----
      The evaluation is carried out using the relation to the incomplete gamma
      integral (regularized gamma function).
  
      Wrapper for the Cephes [1]_ routine `gdtrc`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "gdtria",
      """
      gdtria(p, b, x, out=None)
  
      Inverse of `gdtr` vs a.
  
      Returns the inverse with respect to the parameter `a` of ``p =
      gdtr(a, b, x)``, the cumulative distribution function of the gamma
      distribution.
  
      Parameters
      ----------
      p : array_like
          Probability values.
      b : array_like
          `b` parameter values of `gdtr(a, b, x)`.  `b` is the "shape" parameter
          of the gamma distribution.
      x : array_like
          Nonnegative real values, from the domain of the gamma distribution.
      out : ndarray, optional
          If a fourth argument is given, it must be a numpy.ndarray whose size
          matches the broadcast result of `a`, `b` and `x`.  `out` is then the
          array returned by the function.
  
      Returns
      -------
      a : ndarray
          Values of the `a` parameter such that `p = gdtr(a, b, x)`.  `1/a`
          is the "scale" parameter of the gamma distribution.
  
      See Also
      --------
      gdtr : CDF of the gamma distribution.
      gdtrib : Inverse with respect to `b` of `gdtr(a, b, x)`.
      gdtrix : Inverse with respect to `x` of `gdtr(a, b, x)`.
  
      Notes
      -----
      Wrapper for the CDFLIB [1]_ Fortran routine `cdfgam`.
  
      The cumulative distribution function `p` is computed using a routine by
      DiDinato and Morris [2]_.  Computation of `a` involves a seach for a value
      that produces the desired value of `p`.  The search relies on the
      monotinicity of `p` with `a`.
  
      References
      ----------
      .. [1] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
      .. [2] DiDinato, A. R. and Morris, A. H.,
             Computation of the incomplete gamma function ratios and their
             inverse.  ACM Trans. Math. Softw. 12 (1986), 377-393.
  
      Examples
      --------
      First evaluate `gdtr`.
  
      >>> from scipy.special import gdtr, gdtria
      >>> p = gdtr(1.2, 3.4, 5.6)
      >>> print(p)
      0.94378087442
  
      Verify the inverse.
  
      >>> gdtria(p, 3.4, 5.6)
      1.2
      """)
  
  add_newdoc("scipy.special", "gdtrib",
      """
      gdtrib(a, p, x, out=None)
  
      Inverse of `gdtr` vs b.
  
      Returns the inverse with respect to the parameter `b` of ``p =
      gdtr(a, b, x)``, the cumulative distribution function of the gamma
      distribution.
  
      Parameters
      ----------
      a : array_like
          `a` parameter values of `gdtr(a, b, x)`. `1/a` is the "scale"
          parameter of the gamma distribution.
      p : array_like
          Probability values.
      x : array_like
          Nonnegative real values, from the domain of the gamma distribution.
      out : ndarray, optional
          If a fourth argument is given, it must be a numpy.ndarray whose size
          matches the broadcast result of `a`, `b` and `x`.  `out` is then the
          array returned by the function.
  
      Returns
      -------
      b : ndarray
          Values of the `b` parameter such that `p = gdtr(a, b, x)`.  `b` is
          the "shape" parameter of the gamma distribution.
  
      See Also
      --------
      gdtr : CDF of the gamma distribution.
      gdtria : Inverse with respect to `a` of `gdtr(a, b, x)`.
      gdtrix : Inverse with respect to `x` of `gdtr(a, b, x)`.
  
      Notes
      -----
      Wrapper for the CDFLIB [1]_ Fortran routine `cdfgam`.
  
      The cumulative distribution function `p` is computed using a routine by
      DiDinato and Morris [2]_.  Computation of `b` involves a seach for a value
      that produces the desired value of `p`.  The search relies on the
      monotinicity of `p` with `b`.
  
      References
      ----------
      .. [1] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
      .. [2] DiDinato, A. R. and Morris, A. H.,
             Computation of the incomplete gamma function ratios and their
             inverse.  ACM Trans. Math. Softw. 12 (1986), 377-393.
  
      Examples
      --------
      First evaluate `gdtr`.
  
      >>> from scipy.special import gdtr, gdtrib
      >>> p = gdtr(1.2, 3.4, 5.6)
      >>> print(p)
      0.94378087442
  
      Verify the inverse.
  
      >>> gdtrib(1.2, p, 5.6)
      3.3999999999723882
      """)
  
  add_newdoc("scipy.special", "gdtrix",
      """
      gdtrix(a, b, p, out=None)
  
      Inverse of `gdtr` vs x.
  
      Returns the inverse with respect to the parameter `x` of ``p =
      gdtr(a, b, x)``, the cumulative distribution function of the gamma
      distribution. This is also known as the p'th quantile of the
      distribution.
  
      Parameters
      ----------
      a : array_like
          `a` parameter values of `gdtr(a, b, x)`.  `1/a` is the "scale"
          parameter of the gamma distribution.
      b : array_like
          `b` parameter values of `gdtr(a, b, x)`.  `b` is the "shape" parameter
          of the gamma distribution.
      p : array_like
          Probability values.
      out : ndarray, optional
          If a fourth argument is given, it must be a numpy.ndarray whose size
          matches the broadcast result of `a`, `b` and `x`.  `out` is then the
          array returned by the function.
  
      Returns
      -------
      x : ndarray
          Values of the `x` parameter such that `p = gdtr(a, b, x)`.
  
      See Also
      --------
      gdtr : CDF of the gamma distribution.
      gdtria : Inverse with respect to `a` of `gdtr(a, b, x)`.
      gdtrib : Inverse with respect to `b` of `gdtr(a, b, x)`.
  
      Notes
      -----
      Wrapper for the CDFLIB [1]_ Fortran routine `cdfgam`.
  
      The cumulative distribution function `p` is computed using a routine by
      DiDinato and Morris [2]_.  Computation of `x` involves a seach for a value
      that produces the desired value of `p`.  The search relies on the
      monotinicity of `p` with `x`.
  
      References
      ----------
      .. [1] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
      .. [2] DiDinato, A. R. and Morris, A. H.,
             Computation of the incomplete gamma function ratios and their
             inverse.  ACM Trans. Math. Softw. 12 (1986), 377-393.
  
      Examples
      --------
      First evaluate `gdtr`.
  
      >>> from scipy.special import gdtr, gdtrix
      >>> p = gdtr(1.2, 3.4, 5.6)
      >>> print(p)
      0.94378087442
  
      Verify the inverse.
  
      >>> gdtrix(1.2, 3.4, p)
      5.5999999999999996
      """)
  
  add_newdoc("scipy.special", "hankel1",
      r"""
      hankel1(v, z)
  
      Hankel function of the first kind
  
      Parameters
      ----------
      v : array_like
          Order (float).
      z : array_like
          Argument (float or complex).
  
      Returns
      -------
      out : Values of the Hankel function of the first kind.
  
      Notes
      -----
      A wrapper for the AMOS [1]_ routine `zbesh`, which carries out the
      computation using the relation,
  
      .. math:: H^{(1)}_v(z) = \frac{2}{\imath\pi} \exp(-\imath \pi v/2) K_v(z \exp(-\imath\pi/2))
  
      where :math:`K_v` is the modified Bessel function of the second kind.
      For negative orders, the relation
  
      .. math:: H^{(1)}_{-v}(z) = H^{(1)}_v(z) \exp(\imath\pi v)
  
      is used.
  
      See also
      --------
      hankel1e : this function with leading exponential behavior stripped off.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      """)
  
  add_newdoc("scipy.special", "hankel1e",
      r"""
      hankel1e(v, z)
  
      Exponentially scaled Hankel function of the first kind
  
      Defined as::
  
          hankel1e(v, z) = hankel1(v, z) * exp(-1j * z)
  
      Parameters
      ----------
      v : array_like
          Order (float).
      z : array_like
          Argument (float or complex).
  
      Returns
      -------
      out : Values of the exponentially scaled Hankel function.
  
      Notes
      -----
      A wrapper for the AMOS [1]_ routine `zbesh`, which carries out the
      computation using the relation,
  
      .. math:: H^{(1)}_v(z) = \frac{2}{\imath\pi} \exp(-\imath \pi v/2) K_v(z \exp(-\imath\pi/2))
  
      where :math:`K_v` is the modified Bessel function of the second kind.
      For negative orders, the relation
  
      .. math:: H^{(1)}_{-v}(z) = H^{(1)}_v(z) \exp(\imath\pi v)
  
      is used.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      """)
  
  add_newdoc("scipy.special", "hankel2",
      r"""
      hankel2(v, z)
  
      Hankel function of the second kind
  
      Parameters
      ----------
      v : array_like
          Order (float).
      z : array_like
          Argument (float or complex).
  
      Returns
      -------
      out : Values of the Hankel function of the second kind.
  
      Notes
      -----
      A wrapper for the AMOS [1]_ routine `zbesh`, which carries out the
      computation using the relation,
  
      .. math:: H^{(2)}_v(z) = -\frac{2}{\imath\pi} \exp(\imath \pi v/2) K_v(z \exp(\imath\pi/2))
  
      where :math:`K_v` is the modified Bessel function of the second kind.
      For negative orders, the relation
  
      .. math:: H^{(2)}_{-v}(z) = H^{(2)}_v(z) \exp(-\imath\pi v)
  
      is used.
  
      See also
      --------
      hankel2e : this function with leading exponential behavior stripped off.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      """)
  
  add_newdoc("scipy.special", "hankel2e",
      r"""
      hankel2e(v, z)
  
      Exponentially scaled Hankel function of the second kind
  
      Defined as::
  
          hankel2e(v, z) = hankel2(v, z) * exp(1j * z)
  
      Parameters
      ----------
      v : array_like
          Order (float).
      z : array_like
          Argument (float or complex).
  
      Returns
      -------
      out : Values of the exponentially scaled Hankel function of the second kind.
  
      Notes
      -----
      A wrapper for the AMOS [1]_ routine `zbesh`, which carries out the
      computation using the relation,
  
      .. math:: H^{(2)}_v(z) = -\frac{2}{\imath\pi} \exp(\frac{\imath \pi v}{2}) K_v(z exp(\frac{\imath\pi}{2}))
  
      where :math:`K_v` is the modified Bessel function of the second kind.
      For negative orders, the relation
  
      .. math:: H^{(2)}_{-v}(z) = H^{(2)}_v(z) \exp(-\imath\pi v)
  
      is used.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
  
      """)
  
  add_newdoc("scipy.special", "huber",
      r"""
      huber(delta, r)
  
      Huber loss function.
  
      .. math:: \text{huber}(\delta, r) = \begin{cases} \infty & \delta < 0  \\ \frac{1}{2}r^2 & 0 \le \delta, | r | \le \delta \\ \delta ( |r| - \frac{1}{2}\delta ) & \text{otherwise} \end{cases}
  
      Parameters
      ----------
      delta : ndarray
          Input array, indicating the quadratic vs. linear loss changepoint.
      r : ndarray
          Input array, possibly representing residuals.
  
      Returns
      -------
      res : ndarray
          The computed Huber loss function values.
  
      Notes
      -----
      This function is convex in r.
  
      .. versionadded:: 0.15.0
  
      """)
  
  add_newdoc("scipy.special", "hyp0f1", 
      r"""
      hyp0f1(v, x)
  
      Confluent hypergeometric limit function 0F1.
  
      Parameters
      ----------
      v, z : array_like
          Input values.
  
      Returns
      -------
      hyp0f1 : ndarray
          The confluent hypergeometric limit function.
  
      Notes
      -----
      This function is defined as:
  
      .. math:: _0F_1(v, z) = \sum_{k=0}^{\infty}\frac{z^k}{(v)_k k!}.
  
      It's also the limit as :math:`q \to \infty` of :math:`_1F_1(q; v; z/q)`,
      and satisfies the differential equation :math:`f''(z) + vf'(z) = f(z)`.
      """)
  
  add_newdoc("scipy.special", "hyp1f1",
      """
      hyp1f1(a, b, x)
  
      Confluent hypergeometric function 1F1(a, b; x)
      """)
  
  add_newdoc("scipy.special", "hyp1f2",
      """
      hyp1f2(a, b, c, x)
  
      Hypergeometric function 1F2 and error estimate
  
      Returns
      -------
      y
          Value of the function
      err
          Error estimate
      """)
  
  add_newdoc("scipy.special", "hyp2f0",
      """
      hyp2f0(a, b, x, type)
  
      Hypergeometric function 2F0 in y and an error estimate
  
      The parameter `type` determines a convergence factor and can be
      either 1 or 2.
  
      Returns
      -------
      y
          Value of the function
      err
          Error estimate
      """)
  
  add_newdoc("scipy.special", "hyp2f1",
      """
      hyp2f1(a, b, c, z)
  
      Gauss hypergeometric function 2F1(a, b; c; z).
      """)
  
  add_newdoc("scipy.special", "hyp3f0",
      """
      hyp3f0(a, b, c, x)
  
      Hypergeometric function 3F0 in y and an error estimate
  
      Returns
      -------
      y
          Value of the function
      err
          Error estimate
      """)
  
  add_newdoc("scipy.special", "hyperu",
      """
      hyperu(a, b, x)
  
      Confluent hypergeometric function U(a, b, x) of the second kind
      """)
  
  add_newdoc("scipy.special", "i0",
      r"""
      i0(x)
  
      Modified Bessel function of order 0.
  
      Defined as,
  
      .. math::
          I_0(x) = \sum_{k=0}^\infty \frac{(x^2/4)^k}{(k!)^2} = J_0(\imath x),
  
      where :math:`J_0` is the Bessel function of the first kind of order 0.
  
      Parameters
      ----------
      x : array_like
          Argument (float)
  
      Returns
      -------
      I : ndarray
          Value of the modified Bessel function of order 0 at `x`.
  
      Notes
      -----
      The range is partitioned into the two intervals [0, 8] and (8, infinity).
      Chebyshev polynomial expansions are employed in each interval.
  
      This function is a wrapper for the Cephes [1]_ routine `i0`.
  
      See also
      --------
      iv
      i0e
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "i0e",
      """
      i0e(x)
  
      Exponentially scaled modified Bessel function of order 0.
  
      Defined as::
  
          i0e(x) = exp(-abs(x)) * i0(x).
  
      Parameters
      ----------
      x : array_like
          Argument (float)
  
      Returns
      -------
      I : ndarray
          Value of the exponentially scaled modified Bessel function of order 0
          at `x`.
  
      Notes
      -----
      The range is partitioned into the two intervals [0, 8] and (8, infinity).
      Chebyshev polynomial expansions are employed in each interval.  The
      polynomial expansions used are the same as those in `i0`, but
      they are not multiplied by the dominant exponential factor.
  
      This function is a wrapper for the Cephes [1]_ routine `i0e`.
  
      See also
      --------
      iv
      i0
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "i1",
      r"""
      i1(x)
  
      Modified Bessel function of order 1.
  
      Defined as,
  
      .. math::
          I_1(x) = \frac{1}{2}x \sum_{k=0}^\infty \frac{(x^2/4)^k}{k! (k + 1)!}
                 = -\imath J_1(\imath x),
  
      where :math:`J_1` is the Bessel function of the first kind of order 1.
  
      Parameters
      ----------
      x : array_like
          Argument (float)
  
      Returns
      -------
      I : ndarray
          Value of the modified Bessel function of order 1 at `x`.
  
      Notes
      -----
      The range is partitioned into the two intervals [0, 8] and (8, infinity).
      Chebyshev polynomial expansions are employed in each interval.
  
      This function is a wrapper for the Cephes [1]_ routine `i1`.
  
      See also
      --------
      iv
      i1e
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "i1e",
      """
      i1e(x)
  
      Exponentially scaled modified Bessel function of order 1.
  
      Defined as::
  
          i1e(x) = exp(-abs(x)) * i1(x)
  
      Parameters
      ----------
      x : array_like
          Argument (float)
  
      Returns
      -------
      I : ndarray
          Value of the exponentially scaled modified Bessel function of order 1
          at `x`.
  
      Notes
      -----
      The range is partitioned into the two intervals [0, 8] and (8, infinity).
      Chebyshev polynomial expansions are employed in each interval. The
      polynomial expansions used are the same as those in `i1`, but
      they are not multiplied by the dominant exponential factor.
  
      This function is a wrapper for the Cephes [1]_ routine `i1e`.
  
      See also
      --------
      iv
      i1
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "it2i0k0",
      """
      it2i0k0(x)
  
      Integrals related to modified Bessel functions of order 0
  
      Returns
      -------
      ii0
          ``integral((i0(t)-1)/t, t=0..x)``
      ik0
          ``int(k0(t)/t, t=x..inf)``
      """)
  
  add_newdoc("scipy.special", "it2j0y0",
      """
      it2j0y0(x)
  
      Integrals related to Bessel functions of order 0
  
      Returns
      -------
      ij0
          ``integral((1-j0(t))/t, t=0..x)``
      iy0
          ``integral(y0(t)/t, t=x..inf)``
      """)
  
  add_newdoc("scipy.special", "it2struve0",
      r"""
      it2struve0(x)
  
      Integral related to the Struve function of order 0.
  
      Returns the integral,
  
      .. math::
          \int_x^\infty \frac{H_0(t)}{t}\,dt
  
      where :math:`H_0` is the Struve function of order 0.
  
      Parameters
      ----------
      x : array_like
          Lower limit of integration.
  
      Returns
      -------
      I : ndarray
          The value of the integral.
  
      See also
      --------
      struve
  
      Notes
      -----
      Wrapper for a Fortran routine created by Shanjie Zhang and Jianming
      Jin [1]_.
  
      References
      ----------
      .. [1] Zhang, Shanjie and Jin, Jianming. "Computation of Special
             Functions", John Wiley and Sons, 1996.
             http://jin.ece.illinois.edu/specfunc.html
      """)
  
  add_newdoc("scipy.special", "itairy",
      """
      itairy(x)
  
      Integrals of Airy functions
  
      Calculates the integrals of Airy functions from 0 to `x`.
  
      Parameters
      ----------
  
      x: array_like
          Upper limit of integration (float).
  
      Returns
      -------
      Apt
          Integral of Ai(t) from 0 to x.
      Bpt
          Integral of Bi(t) from 0 to x.
      Ant
          Integral of Ai(-t) from 0 to x.
      Bnt
          Integral of Bi(-t) from 0 to x.
  
      Notes
      -----
  
      Wrapper for a Fortran routine created by Shanjie Zhang and Jianming
      Jin [1]_.
  
      References
      ----------
  
      .. [1] Zhang, Shanjie and Jin, Jianming. "Computation of Special
             Functions", John Wiley and Sons, 1996.
             http://jin.ece.illinois.edu/specfunc.html
      """)
  
  add_newdoc("scipy.special", "iti0k0",
      """
      iti0k0(x)
  
      Integrals of modified Bessel functions of order 0
  
      Returns simple integrals from 0 to `x` of the zeroth order modified
      Bessel functions `i0` and `k0`.
  
      Returns
      -------
      ii0, ik0
      """)
  
  add_newdoc("scipy.special", "itj0y0",
      """
      itj0y0(x)
  
      Integrals of Bessel functions of order 0
  
      Returns simple integrals from 0 to `x` of the zeroth order Bessel
      functions `j0` and `y0`.
  
      Returns
      -------
      ij0, iy0
      """)
  
  add_newdoc("scipy.special", "itmodstruve0",
      r"""
      itmodstruve0(x)
  
      Integral of the modified Struve function of order 0.
  
      .. math::
          I = \int_0^x L_0(t)\,dt
  
      Parameters
      ----------
      x : array_like
          Upper limit of integration (float).
  
      Returns
      -------
      I : ndarray
          The integral of :math:`L_0` from 0 to `x`.
  
      Notes
      -----
      Wrapper for a Fortran routine created by Shanjie Zhang and Jianming
      Jin [1]_.
  
      References
      ----------
      .. [1] Zhang, Shanjie and Jin, Jianming. "Computation of Special
             Functions", John Wiley and Sons, 1996.
             http://jin.ece.illinois.edu/specfunc.html
  
      """)
  
  add_newdoc("scipy.special", "itstruve0",
      r"""
      itstruve0(x)
  
      Integral of the Struve function of order 0.
  
      .. math::
          I = \int_0^x H_0(t)\,dt
  
      Parameters
      ----------
      x : array_like
          Upper limit of integration (float).
  
      Returns
      -------
      I : ndarray
          The integral of :math:`H_0` from 0 to `x`.
  
      See also
      --------
      struve
  
      Notes
      -----
      Wrapper for a Fortran routine created by Shanjie Zhang and Jianming
      Jin [1]_.
  
      References
      ----------
      .. [1] Zhang, Shanjie and Jin, Jianming. "Computation of Special
             Functions", John Wiley and Sons, 1996.
             http://jin.ece.illinois.edu/specfunc.html
  
      """)
  
  add_newdoc("scipy.special", "iv",
      r"""
      iv(v, z)
  
      Modified Bessel function of the first kind of real order.
  
      Parameters
      ----------
      v : array_like
          Order. If `z` is of real type and negative, `v` must be integer
          valued.
      z : array_like of float or complex
          Argument.
  
      Returns
      -------
      out : ndarray
          Values of the modified Bessel function.
  
      Notes
      -----
      For real `z` and :math:`v \in [-50, 50]`, the evaluation is carried out
      using Temme's method [1]_.  For larger orders, uniform asymptotic
      expansions are applied.
  
      For complex `z` and positive `v`, the AMOS [2]_ `zbesi` routine is
      called. It uses a power series for small `z`, the asymptitic expansion
      for large `abs(z)`, the Miller algorithm normalized by the Wronskian
      and a Neumann series for intermediate magnitudes, and the uniform
      asymptitic expansions for :math:`I_v(z)` and :math:`J_v(z)` for large
      orders.  Backward recurrence is used to generate sequences or reduce
      orders when necessary.
  
      The calculations above are done in the right half plane and continued
      into the left half plane by the formula,
  
      .. math:: I_v(z \exp(\pm\imath\pi)) = \exp(\pm\pi v) I_v(z)
  
      (valid when the real part of `z` is positive).  For negative `v`, the
      formula
  
      .. math:: I_{-v}(z) = I_v(z) + \frac{2}{\pi} \sin(\pi v) K_v(z)
  
      is used, where :math:`K_v(z)` is the modified Bessel function of the
      second kind, evaluated using the AMOS routine `zbesk`.
  
      See also
      --------
      kve : This function with leading exponential behavior stripped off.
  
      References
      ----------
      .. [1] Temme, Journal of Computational Physics, vol 21, 343 (1976)
      .. [2] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      """)
  
  add_newdoc("scipy.special", "ive",
      r"""
      ive(v, z)
  
      Exponentially scaled modified Bessel function of the first kind
  
      Defined as::
  
          ive(v, z) = iv(v, z) * exp(-abs(z.real))
  
      Parameters
      ----------
      v : array_like of float
          Order.
      z : array_like of float or complex
          Argument.
  
      Returns
      -------
      out : ndarray
          Values of the exponentially scaled modified Bessel function.
  
      Notes
      -----
      For positive `v`, the AMOS [1]_ `zbesi` routine is called. It uses a
      power series for small `z`, the asymptitic expansion for large
      `abs(z)`, the Miller algorithm normalized by the Wronskian and a
      Neumann series for intermediate magnitudes, and the uniform asymptitic
      expansions for :math:`I_v(z)` and :math:`J_v(z)` for large orders.
      Backward recurrence is used to generate sequences or reduce orders when
      necessary.
  
      The calculations above are done in the right half plane and continued
      into the left half plane by the formula,
  
      .. math:: I_v(z \exp(\pm\imath\pi)) = \exp(\pm\pi v) I_v(z)
  
      (valid when the real part of `z` is positive).  For negative `v`, the
      formula
  
      .. math:: I_{-v}(z) = I_v(z) + \frac{2}{\pi} \sin(\pi v) K_v(z)
  
      is used, where :math:`K_v(z)` is the modified Bessel function of the
      second kind, evaluated using the AMOS routine `zbesk`.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      """)
  
  add_newdoc("scipy.special", "j0",
      r"""
      j0(x)
  
      Bessel function of the first kind of order 0.
  
      Parameters
      ----------
      x : array_like
          Argument (float).
  
      Returns
      -------
      J : ndarray
          Value of the Bessel function of the first kind of order 0 at `x`.
  
      Notes
      -----
      The domain is divided into the intervals [0, 5] and (5, infinity). In the
      first interval the following rational approximation is used:
  
      .. math::
  
          J_0(x) \approx (w - r_1^2)(w - r_2^2) \frac{P_3(w)}{Q_8(w)},
  
      where :math:`w = x^2` and :math:`r_1`, :math:`r_2` are the zeros of
      :math:`J_0`, and :math:`P_3` and :math:`Q_8` are polynomials of degrees 3
      and 8, respectively.
  
      In the second interval, the Hankel asymptotic expansion is employed with
      two rational functions of degree 6/6 and 7/7.
  
      This function is a wrapper for the Cephes [1]_ routine `j0`.
  
      See also
      --------
      jv : Bessel function of real order and complex argument.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "j1",
      """
      j1(x)
  
      Bessel function of the first kind of order 1.
  
      Parameters
      ----------
      x : array_like
          Argument (float).
  
      Returns
      -------
      J : ndarray
          Value of the Bessel function of the first kind of order 1 at `x`.
  
      Notes
      -----
      The domain is divided into the intervals [0, 8] and (8, infinity). In the
      first interval a 24 term Chebyshev expansion is used. In the second, the
      asymptotic trigonometric representation is employed using two rational
      functions of degree 5/5.
  
      This function is a wrapper for the Cephes [1]_ routine `j1`.
  
      See also
      --------
      jv
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "jn",
      """
      jn(n, x)
  
      Bessel function of the first kind of integer order and real argument.
  
      Notes
      -----
      `jn` is an alias of `jv`.
  
      See also
      --------
      jv
  
      """)
  
  add_newdoc("scipy.special", "jv",
      r"""
      jv(v, z)
  
      Bessel function of the first kind of real order and complex argument.
  
      Parameters
      ----------
      v : array_like
          Order (float).
      z : array_like
          Argument (float or complex).
  
      Returns
      -------
      J : ndarray
          Value of the Bessel function, :math:`J_v(z)`.
  
      Notes
      -----
      For positive `v` values, the computation is carried out using the AMOS
      [1]_ `zbesj` routine, which exploits the connection to the modified
      Bessel function :math:`I_v`,
  
      .. math::
          J_v(z) = \exp(n\pi\imath/2) I_v(-\imath z)\qquad (\Im z > 0)
  
          J_v(z) = \exp(-n\pi\imath/2) I_v(\imath z)\qquad (\Im z < 0)
  
      For negative `v` values the formula,
  
      .. math:: J_{-v}(z) = J_v(z) \cos(\pi v) - Y_v(z) \sin(\pi v)
  
      is used, where :math:`Y_v(z)` is the Bessel function of the second
      kind, computed using the AMOS routine `zbesy`.  Note that the second
      term is exactly zero for integer `v`; to improve accuracy the second
      term is explicitly omitted for `v` values such that `v = floor(v)`.
  
      See also
      --------
      jve : :math:`J_v` with leading exponential behavior stripped off.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      """)
  
  add_newdoc("scipy.special", "jve",
      r"""
      jve(v, z)
  
      Exponentially scaled Bessel function of order `v`.
  
      Defined as::
  
          jve(v, z) = jv(v, z) * exp(-abs(z.imag))
  
      Parameters
      ----------
      v : array_like
          Order (float).
      z : array_like
          Argument (float or complex).
  
      Returns
      -------
      J : ndarray
          Value of the exponentially scaled Bessel function.
  
      Notes
      -----
      For positive `v` values, the computation is carried out using the AMOS
      [1]_ `zbesj` routine, which exploits the connection to the modified
      Bessel function :math:`I_v`,
  
      .. math::
          J_v(z) = \exp(n\pi\imath/2) I_v(-\imath z)\qquad (\Im z > 0)
  
          J_v(z) = \exp(-n\pi\imath/2) I_v(\imath z)\qquad (\Im z < 0)
  
      For negative `v` values the formula,
  
      .. math:: J_{-v}(z) = J_v(z) \cos(\pi v) - Y_v(z) \sin(\pi v)
  
      is used, where :math:`Y_v(z)` is the Bessel function of the second
      kind, computed using the AMOS routine `zbesy`.  Note that the second
      term is exactly zero for integer `v`; to improve accuracy the second
      term is explicitly omitted for `v` values such that `v = floor(v)`.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      """)
  
  add_newdoc("scipy.special", "k0",
      r"""
      k0(x)
  
      Modified Bessel function of the second kind of order 0, :math:`K_0`.
  
      This function is also sometimes referred to as the modified Bessel
      function of the third kind of order 0.
  
      Parameters
      ----------
      x : array_like
          Argument (float).
  
      Returns
      -------
      K : ndarray
          Value of the modified Bessel function :math:`K_0` at `x`.
  
      Notes
      -----
      The range is partitioned into the two intervals [0, 2] and (2, infinity).
      Chebyshev polynomial expansions are employed in each interval.
  
      This function is a wrapper for the Cephes [1]_ routine `k0`.
  
      See also
      --------
      kv
      k0e
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "k0e",
      """
      k0e(x)
  
      Exponentially scaled modified Bessel function K of order 0
  
      Defined as::
  
          k0e(x) = exp(x) * k0(x).
  
      Parameters
      ----------
      x : array_like
          Argument (float)
  
      Returns
      -------
      K : ndarray
          Value of the exponentially scaled modified Bessel function K of order
          0 at `x`.
  
      Notes
      -----
      The range is partitioned into the two intervals [0, 2] and (2, infinity).
      Chebyshev polynomial expansions are employed in each interval.
  
      This function is a wrapper for the Cephes [1]_ routine `k0e`.
  
      See also
      --------
      kv
      k0
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "k1",
      """
      k1(x)
  
      Modified Bessel function of the second kind of order 1, :math:`K_1(x)`.
  
      Parameters
      ----------
      x : array_like
          Argument (float)
  
      Returns
      -------
      K : ndarray
          Value of the modified Bessel function K of order 1 at `x`.
  
      Notes
      -----
      The range is partitioned into the two intervals [0, 2] and (2, infinity).
      Chebyshev polynomial expansions are employed in each interval.
  
      This function is a wrapper for the Cephes [1]_ routine `k1`.
  
      See also
      --------
      kv
      k1e
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "k1e",
      """
      k1e(x)
  
      Exponentially scaled modified Bessel function K of order 1
  
      Defined as::
  
          k1e(x) = exp(x) * k1(x)
  
      Parameters
      ----------
      x : array_like
          Argument (float)
  
      Returns
      -------
      K : ndarray
          Value of the exponentially scaled modified Bessel function K of order
          1 at `x`.
  
      Notes
      -----
      The range is partitioned into the two intervals [0, 2] and (2, infinity).
      Chebyshev polynomial expansions are employed in each interval.
  
      This function is a wrapper for the Cephes [1]_ routine `k1e`.
  
      See also
      --------
      kv
      k1
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "kei",
      """
      kei(x)
  
      Kelvin function ker
      """)
  
  add_newdoc("scipy.special", "keip",
      """
      keip(x)
  
      Derivative of the Kelvin function kei
      """)
  
  add_newdoc("scipy.special", "kelvin",
      """
      kelvin(x)
  
      Kelvin functions as complex numbers
  
      Returns
      -------
      Be, Ke, Bep, Kep
          The tuple (Be, Ke, Bep, Kep) contains complex numbers
          representing the real and imaginary Kelvin functions and their
          derivatives evaluated at `x`.  For example, kelvin(x)[0].real =
          ber x and kelvin(x)[0].imag = bei x with similar relationships
          for ker and kei.
      """)
  
  add_newdoc("scipy.special", "ker",
      """
      ker(x)
  
      Kelvin function ker
      """)
  
  add_newdoc("scipy.special", "kerp",
      """
      kerp(x)
  
      Derivative of the Kelvin function ker
      """)
  
  add_newdoc("scipy.special", "kl_div",
      r"""
      kl_div(x, y)
  
      Elementwise function for computing Kullback-Leibler divergence.
  
      .. math:: \mathrm{kl\_div}(x, y) = \begin{cases} x \log(x / y) - x + y & x > 0, y > 0 \\ y & x = 0, y \ge 0 \\ \infty & \text{otherwise} \end{cases}
  
      Parameters
      ----------
      x : ndarray
          First input array.
      y : ndarray
          Second input array.
  
      Returns
      -------
      res : ndarray
          Output array.
  
      See Also
      --------
      entr, rel_entr
  
      Notes
      -----
      This function is non-negative and is jointly convex in `x` and `y`.
  
      .. versionadded:: 0.15.0
  
      """)
  
  add_newdoc("scipy.special", "kn",
      r"""
      kn(n, x)
  
      Modified Bessel function of the second kind of integer order `n`
  
      Returns the modified Bessel function of the second kind for integer order
      `n` at real `z`.
  
      These are also sometimes called functions of the third kind, Basset
      functions, or Macdonald functions.
  
      Parameters
      ----------
      n : array_like of int
          Order of Bessel functions (floats will truncate with a warning)
      z : array_like of float
          Argument at which to evaluate the Bessel functions
  
      Returns
      -------
      out : ndarray
          The results
  
      Notes
      -----
      Wrapper for AMOS [1]_ routine `zbesk`.  For a discussion of the
      algorithm used, see [2]_ and the references therein.
  
      See Also
      --------
      kv : Same function, but accepts real order and complex argument
      kvp : Derivative of this function
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      .. [2] Donald E. Amos, "Algorithm 644: A portable package for Bessel
             functions of a complex argument and nonnegative order", ACM
             TOMS Vol. 12 Issue 3, Sept. 1986, p. 265
  
      Examples
      --------
      Plot the function of several orders for real input:
  
      >>> from scipy.special import kn
      >>> import matplotlib.pyplot as plt
      >>> x = np.linspace(0, 5, 1000)
      >>> for N in range(6):
      ...     plt.plot(x, kn(N, x), label='$K_{}(x)$'.format(N))
      >>> plt.ylim(0, 10)
      >>> plt.legend()
      >>> plt.title(r'Modified Bessel function of the second kind $K_n(x)$')
      >>> plt.show()
  
      Calculate for a single value at multiple orders:
  
      >>> kn([4, 5, 6], 1)
      array([   44.23241585,   360.9605896 ,  3653.83831186])
      """)
  
  add_newdoc("scipy.special", "kolmogi",
      """
      kolmogi(p)
  
      Inverse function to kolmogorov
  
      Returns y such that ``kolmogorov(y) == p``.
      """)
  
  add_newdoc("scipy.special", "kolmogorov",
      """
      kolmogorov(y)
  
      Complementary cumulative distribution function of Kolmogorov distribution
  
      Returns the complementary cumulative distribution function of
      Kolmogorov's limiting distribution (Kn* for large n) of a
      two-sided test for equality between an empirical and a theoretical
      distribution. It is equal to the (limit as n->infinity of the)
      probability that sqrt(n) * max absolute deviation > y.
      """)
  
  add_newdoc("scipy.special", "kv",
      r"""
      kv(v, z)
  
      Modified Bessel function of the second kind of real order `v`
  
      Returns the modified Bessel function of the second kind for real order
      `v` at complex `z`.
  
      These are also sometimes called functions of the third kind, Basset
      functions, or Macdonald functions.  They are defined as those solutions
      of the modified Bessel equation for which,
  
      .. math::
          K_v(x) \sim \sqrt{\pi/(2x)} \exp(-x)
  
      as :math:`x \to \infty` [3]_.
  
      Parameters
      ----------
      v : array_like of float
          Order of Bessel functions
      z : array_like of complex
          Argument at which to evaluate the Bessel functions
  
      Returns
      -------
      out : ndarray
          The results. Note that input must be of complex type to get complex
          output, e.g. ``kv(3, -2+0j)`` instead of ``kv(3, -2)``.
  
      Notes
      -----
      Wrapper for AMOS [1]_ routine `zbesk`.  For a discussion of the
      algorithm used, see [2]_ and the references therein.
  
      See Also
      --------
      kve : This function with leading exponential behavior stripped off.
      kvp : Derivative of this function
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      .. [2] Donald E. Amos, "Algorithm 644: A portable package for Bessel
             functions of a complex argument and nonnegative order", ACM
             TOMS Vol. 12 Issue 3, Sept. 1986, p. 265
      .. [3] NIST Digital Library of Mathematical Functions,
             Eq. 10.25.E3. http://dlmf.nist.gov/10.25.E3
  
      Examples
      --------
      Plot the function of several orders for real input:
  
      >>> from scipy.special import kv
      >>> import matplotlib.pyplot as plt
      >>> x = np.linspace(0, 5, 1000)
      >>> for N in np.linspace(0, 6, 5):
      ...     plt.plot(x, kv(N, x), label='$K_{{{}}}(x)$'.format(N))
      >>> plt.ylim(0, 10)
      >>> plt.legend()
      >>> plt.title(r'Modified Bessel function of the second kind $K_\nu(x)$')
      >>> plt.show()
  
      Calculate for a single value at multiple orders:
  
      >>> kv([4, 4.5, 5], 1+2j)
      array([ 0.1992+2.3892j,  2.3493+3.6j   ,  7.2827+3.8104j])
  
      """)
  
  add_newdoc("scipy.special", "kve",
      r"""
      kve(v, z)
  
      Exponentially scaled modified Bessel function of the second kind.
  
      Returns the exponentially scaled, modified Bessel function of the
      second kind (sometimes called the third kind) for real order `v` at
      complex `z`::
  
          kve(v, z) = kv(v, z) * exp(z)
  
      Parameters
      ----------
      v : array_like of float
          Order of Bessel functions
      z : array_like of complex
          Argument at which to evaluate the Bessel functions
  
      Returns
      -------
      out : ndarray
          The exponentially scaled modified Bessel function of the second kind.
  
      Notes
      -----
      Wrapper for AMOS [1]_ routine `zbesk`.  For a discussion of the
      algorithm used, see [2]_ and the references therein.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      .. [2] Donald E. Amos, "Algorithm 644: A portable package for Bessel
             functions of a complex argument and nonnegative order", ACM
             TOMS Vol. 12 Issue 3, Sept. 1986, p. 265
      """)
  
  add_newdoc("scipy.special", "log1p",
      """
      log1p(x)
  
      Calculates log(1+x) for use when `x` is near zero
      """)
  
  add_newdoc('scipy.special', 'logit',
      """
      logit(x)
  
      Logit ufunc for ndarrays.
  
      The logit function is defined as logit(p) = log(p/(1-p)).
      Note that logit(0) = -inf, logit(1) = inf, and logit(p)
      for p<0 or p>1 yields nan.
  
      Parameters
      ----------
      x : ndarray
          The ndarray to apply logit to element-wise.
  
      Returns
      -------
      out : ndarray
          An ndarray of the same shape as x. Its entries
          are logit of the corresponding entry of x.
  
      Notes
      -----
      As a ufunc logit takes a number of optional
      keyword arguments. For more information
      see `ufuncs <https://docs.scipy.org/doc/numpy/reference/ufuncs.html>`_
  
      .. versionadded:: 0.10.0
  
      """)
  
  add_newdoc("scipy.special", "lpmv",
      """
      lpmv(m, v, x)
  
      Associated legendre function of integer order.
  
      Parameters
      ----------
      m : int
          Order
      v : float
          Degree.
      x : float
          Argument. Must be ``|x| <= 1``.
  
      Returns
      -------
      res : float
          The value of the function.
  
      See Also
      --------
      lpmn : Similar, but computes values for all orders 0..m and degrees 0..n.
      clpmn : Similar to `lpmn` but allows a complex argument.
  
      Notes
      -----
      It is possible to extend the domain of this function to all
      complex m, v, x, but this is not yet implemented.
  
      """)
  
  add_newdoc("scipy.special", "mathieu_a",
      """
      mathieu_a(m, q)
  
      Characteristic value of even Mathieu functions
  
      Returns the characteristic value for the even solution,
      ``ce_m(z, q)``, of Mathieu's equation.
      """)
  
  add_newdoc("scipy.special", "mathieu_b",
      """
      mathieu_b(m, q)
  
      Characteristic value of odd Mathieu functions
  
      Returns the characteristic value for the odd solution,
      ``se_m(z, q)``, of Mathieu's equation.
      """)
  
  add_newdoc("scipy.special", "mathieu_cem",
      """
      mathieu_cem(m, q, x)
  
      Even Mathieu function and its derivative
  
      Returns the even Mathieu function, ``ce_m(x, q)``, of order `m` and
      parameter `q` evaluated at `x` (given in degrees).  Also returns the
      derivative with respect to `x` of ce_m(x, q)
  
      Parameters
      ----------
      m
          Order of the function
      q
          Parameter of the function
      x
          Argument of the function, *given in degrees, not radians*
  
      Returns
      -------
      y
          Value of the function
      yp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "mathieu_modcem1",
      """
      mathieu_modcem1(m, q, x)
  
      Even modified Mathieu function of the first kind and its derivative
  
      Evaluates the even modified Mathieu function of the first kind,
      ``Mc1m(x, q)``, and its derivative at `x` for order `m` and parameter
      `q`.
  
      Returns
      -------
      y
          Value of the function
      yp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "mathieu_modcem2",
      """
      mathieu_modcem2(m, q, x)
  
      Even modified Mathieu function of the second kind and its derivative
  
      Evaluates the even modified Mathieu function of the second kind,
      Mc2m(x, q), and its derivative at `x` (given in degrees) for order `m`
      and parameter `q`.
  
      Returns
      -------
      y
          Value of the function
      yp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "mathieu_modsem1",
      """
      mathieu_modsem1(m, q, x)
  
      Odd modified Mathieu function of the first kind and its derivative
  
      Evaluates the odd modified Mathieu function of the first kind,
      Ms1m(x, q), and its derivative at `x` (given in degrees) for order `m`
      and parameter `q`.
  
      Returns
      -------
      y
          Value of the function
      yp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "mathieu_modsem2",
      """
      mathieu_modsem2(m, q, x)
  
      Odd modified Mathieu function of the second kind and its derivative
  
      Evaluates the odd modified Mathieu function of the second kind,
      Ms2m(x, q), and its derivative at `x` (given in degrees) for order `m`
      and parameter q.
  
      Returns
      -------
      y
          Value of the function
      yp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "mathieu_sem",
      """
      mathieu_sem(m, q, x)
  
      Odd Mathieu function and its derivative
  
      Returns the odd Mathieu function, se_m(x, q), of order `m` and
      parameter `q` evaluated at `x` (given in degrees).  Also returns the
      derivative with respect to `x` of se_m(x, q).
  
      Parameters
      ----------
      m
          Order of the function
      q
          Parameter of the function
      x
          Argument of the function, *given in degrees, not radians*.
  
      Returns
      -------
      y
          Value of the function
      yp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "modfresnelm",
      """
      modfresnelm(x)
  
      Modified Fresnel negative integrals
  
      Returns
      -------
      fm
          Integral ``F_-(x)``: ``integral(exp(-1j*t*t), t=x..inf)``
      km
          Integral ``K_-(x)``: ``1/sqrt(pi)*exp(1j*(x*x+pi/4))*fp``
      """)
  
  add_newdoc("scipy.special", "modfresnelp",
      """
      modfresnelp(x)
  
      Modified Fresnel positive integrals
  
      Returns
      -------
      fp
          Integral ``F_+(x)``: ``integral(exp(1j*t*t), t=x..inf)``
      kp
          Integral ``K_+(x)``: ``1/sqrt(pi)*exp(-1j*(x*x+pi/4))*fp``
      """)
  
  add_newdoc("scipy.special", "modstruve",
      r"""
      modstruve(v, x)
  
      Modified Struve function.
  
      Return the value of the modified Struve function of order `v` at `x`.  The
      modified Struve function is defined as,
  
      .. math::
          L_v(x) = -\imath \exp(-\pi\imath v/2) H_v(x),
  
      where :math:`H_v` is the Struve function.
  
      Parameters
      ----------
      v : array_like
          Order of the modified Struve function (float).
      x : array_like
          Argument of the Struve function (float; must be positive unless `v` is
          an integer).
  
      Returns
      -------
      L : ndarray
          Value of the modified Struve function of order `v` at `x`.
  
      Notes
      -----
      Three methods discussed in [1]_ are used to evaluate the function:
  
      - power series
      - expansion in Bessel functions (if :math:`|z| < |v| + 20`)
      - asymptotic large-z expansion (if :math:`z \geq 0.7v + 12`)
  
      Rounding errors are estimated based on the largest terms in the sums, and
      the result associated with the smallest error is returned.
  
      See also
      --------
      struve
  
      References
      ----------
      .. [1] NIST Digital Library of Mathematical Functions
             http://dlmf.nist.gov/11
      """)
  
  add_newdoc("scipy.special", "nbdtr",
      r"""
      nbdtr(k, n, p)
  
      Negative binomial cumulative distribution function.
  
      Returns the sum of the terms 0 through `k` of the negative binomial
      distribution probability mass function,
  
      .. math::
  
          F = \sum_{j=0}^k {{n + j - 1}\choose{j}} p^n (1 - p)^j.
  
      In a sequence of Bernoulli trials with individual success probabilities
      `p`, this is the probability that `k` or fewer failures precede the nth
      success.
  
      Parameters
      ----------
      k : array_like
          The maximum number of allowed failures (nonnegative int).
      n : array_like
          The target number of successes (positive int).
      p : array_like
          Probability of success in a single event (float).
  
      Returns
      -------
      F : ndarray
          The probability of `k` or fewer failures before `n` successes in a
          sequence of events with individual success probability `p`.
  
      See also
      --------
      nbdtrc
  
      Notes
      -----
      If floating point values are passed for `k` or `n`, they will be truncated
      to integers.
  
      The terms are not summed directly; instead the regularized incomplete beta
      function is employed, according to the formula,
  
      .. math::
          \mathrm{nbdtr}(k, n, p) = I_{p}(n, k + 1).
  
      Wrapper for the Cephes [1]_ routine `nbdtr`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
  
      """)
  
  add_newdoc("scipy.special", "nbdtrc",
      r"""
      nbdtrc(k, n, p)
  
      Negative binomial survival function.
  
      Returns the sum of the terms `k + 1` to infinity of the negative binomial
      distribution probability mass function,
  
      .. math::
  
          F = \sum_{j=k + 1}^\infty {{n + j - 1}\choose{j}} p^n (1 - p)^j.
  
      In a sequence of Bernoulli trials with individual success probabilities
      `p`, this is the probability that more than `k` failures precede the nth
      success.
  
      Parameters
      ----------
      k : array_like
          The maximum number of allowed failures (nonnegative int).
      n : array_like
          The target number of successes (positive int).
      p : array_like
          Probability of success in a single event (float).
  
      Returns
      -------
      F : ndarray
          The probability of `k + 1` or more failures before `n` successes in a
          sequence of events with individual success probability `p`.
  
      Notes
      -----
      If floating point values are passed for `k` or `n`, they will be truncated
      to integers.
  
      The terms are not summed directly; instead the regularized incomplete beta
      function is employed, according to the formula,
  
      .. math::
          \mathrm{nbdtrc}(k, n, p) = I_{1 - p}(k + 1, n).
  
      Wrapper for the Cephes [1]_ routine `nbdtrc`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "nbdtri",
      """
      nbdtri(k, n, y)
  
      Inverse of `nbdtr` vs `p`.
  
      Returns the inverse with respect to the parameter `p` of
      `y = nbdtr(k, n, p)`, the negative binomial cumulative distribution
      function.
  
      Parameters
      ----------
      k : array_like
          The maximum number of allowed failures (nonnegative int).
      n : array_like
          The target number of successes (positive int).
      y : array_like
          The probability of `k` or fewer failures before `n` successes (float).
  
      Returns
      -------
      p : ndarray
          Probability of success in a single event (float) such that
          `nbdtr(k, n, p) = y`.
  
      See also
      --------
      nbdtr : Cumulative distribution function of the negative binomial.
      nbdtrik : Inverse with respect to `k` of `nbdtr(k, n, p)`.
      nbdtrin : Inverse with respect to `n` of `nbdtr(k, n, p)`.
  
      Notes
      -----
      Wrapper for the Cephes [1]_ routine `nbdtri`.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      
      """)
  
  add_newdoc("scipy.special", "nbdtrik",
      r"""
      nbdtrik(y, n, p)
  
      Inverse of `nbdtr` vs `k`.
  
      Returns the inverse with respect to the parameter `k` of
      `y = nbdtr(k, n, p)`, the negative binomial cumulative distribution
      function.
  
      Parameters
      ----------
      y : array_like
          The probability of `k` or fewer failures before `n` successes (float).
      n : array_like
          The target number of successes (positive int).
      p : array_like
          Probability of success in a single event (float).
      
      Returns
      -------
      k : ndarray
          The maximum number of allowed failures such that `nbdtr(k, n, p) = y`.
      
      See also
      --------
      nbdtr : Cumulative distribution function of the negative binomial.
      nbdtri : Inverse with respect to `p` of `nbdtr(k, n, p)`.
      nbdtrin : Inverse with respect to `n` of `nbdtr(k, n, p)`.
  
      Notes
      -----
      Wrapper for the CDFLIB [1]_ Fortran routine `cdfnbn`.
  
      Formula 26.5.26 of [2]_,
  
      .. math::
          \sum_{j=k + 1}^\infty {{n + j - 1}\choose{j}} p^n (1 - p)^j = I_{1 - p}(k + 1, n),
  
      is used to reduce calculation of the cumulative distribution function to
      that of a regularized incomplete beta :math:`I`.
  
      Computation of `k` involves a seach for a value that produces the desired
      value of `y`.  The search relies on the monotinicity of `y` with `k`.
  
      References
      ----------
      .. [1] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
      .. [2] Milton Abramowitz and Irene A. Stegun, eds.
             Handbook of Mathematical Functions with Formulas,
             Graphs, and Mathematical Tables. New York: Dover, 1972.
  
      """)
  
  add_newdoc("scipy.special", "nbdtrin",
      r"""
      nbdtrin(k, y, p)
  
      Inverse of `nbdtr` vs `n`.
  
      Returns the inverse with respect to the parameter `n` of
      `y = nbdtr(k, n, p)`, the negative binomial cumulative distribution
      function.
  
      Parameters
      ----------
      k : array_like
          The maximum number of allowed failures (nonnegative int).
      y : array_like
          The probability of `k` or fewer failures before `n` successes (float).
      p : array_like
          Probability of success in a single event (float).
      
      Returns
      -------
      n : ndarray
          The number of successes `n` such that `nbdtr(k, n, p) = y`.
      
      See also
      --------
      nbdtr : Cumulative distribution function of the negative binomial.
      nbdtri : Inverse with respect to `p` of `nbdtr(k, n, p)`.
      nbdtrik : Inverse with respect to `k` of `nbdtr(k, n, p)`.
  
      Notes
      -----
      Wrapper for the CDFLIB [1]_ Fortran routine `cdfnbn`.
  
      Formula 26.5.26 of [2]_,
  
      .. math::
          \sum_{j=k + 1}^\infty {{n + j - 1}\choose{j}} p^n (1 - p)^j = I_{1 - p}(k + 1, n),
  
      is used to reduce calculation of the cumulative distribution function to
      that of a regularized incomplete beta :math:`I`.
  
      Computation of `n` involves a seach for a value that produces the desired
      value of `y`.  The search relies on the monotinicity of `y` with `n`.
  
      References
      ----------
      .. [1] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
      .. [2] Milton Abramowitz and Irene A. Stegun, eds.
             Handbook of Mathematical Functions with Formulas,
             Graphs, and Mathematical Tables. New York: Dover, 1972.
  
      """)
  
  add_newdoc("scipy.special", "ncfdtr",
      r"""
      ncfdtr(dfn, dfd, nc, f)
  
      Cumulative distribution function of the non-central F distribution.
  
      The non-central F describes the distribution of,
  
      .. math::
          Z = \frac{X/d_n}{Y/d_d}
  
      where :math:`X` and :math:`Y` are independently distributed, with
      :math:`X` distributed non-central :math:`\chi^2` with noncentrality
      parameter `nc` and :math:`d_n` degrees of freedom, and :math:`Y`
      distributed :math:`\chi^2` with :math:`d_d` degrees of freedom.
  
      Parameters
      ----------
      dfn : array_like
          Degrees of freedom of the numerator sum of squares.  Range (0, inf).
      dfd : array_like
          Degrees of freedom of the denominator sum of squares.  Range (0, inf).
      nc : array_like
          Noncentrality parameter.  Should be in range (0, 1e4).
      f : array_like
          Quantiles, i.e. the upper limit of integration.
  
      Returns
      -------
      cdf : float or ndarray
          The calculated CDF.  If all inputs are scalar, the return will be a
          float.  Otherwise it will be an array.
  
      See Also
      --------
      ncdfdtri : Inverse CDF (iCDF) of the non-central F distribution.
      ncdfdtridfd : Calculate dfd, given CDF and iCDF values.
      ncdfdtridfn : Calculate dfn, given CDF and iCDF values.
      ncdfdtrinc : Calculate noncentrality parameter, given CDF, iCDF, dfn, dfd.
  
      Notes
      -----
      Wrapper for the CDFLIB [1]_ Fortran routine `cdffnc`.
  
      The cumulative distribution function is computed using Formula 26.6.20 of
      [2]_:
  
      .. math::
          F(d_n, d_d, n_c, f) = \sum_{j=0}^\infty e^{-n_c/2} \frac{(n_c/2)^j}{j!} I_{x}(\frac{d_n}{2} + j, \frac{d_d}{2}),
  
      where :math:`I` is the regularized incomplete beta function, and
      :math:`x = f d_n/(f d_n + d_d)`.
  
      The computation time required for this routine is proportional to the
      noncentrality parameter `nc`.  Very large values of this parameter can
      consume immense computer resources.  This is why the search range is
      bounded by 10,000.
  
      References
      ----------
      .. [1] Barry Brown, James Lovato, and Kathy Russell,
             CDFLIB: Library of Fortran Routines for Cumulative Distribution
             Functions, Inverses, and Other Parameters.
      .. [2] Milton Abramowitz and Irene A. Stegun, eds.
             Handbook of Mathematical Functions with Formulas,
             Graphs, and Mathematical Tables. New York: Dover, 1972.
  
      Examples
      --------
      >>> from scipy import special
      >>> from scipy import stats
      >>> import matplotlib.pyplot as plt
  
      Plot the CDF of the non-central F distribution, for nc=0.  Compare with the
      F-distribution from scipy.stats:
  
      >>> x = np.linspace(-1, 8, num=500)
      >>> dfn = 3
      >>> dfd = 2
      >>> ncf_stats = stats.f.cdf(x, dfn, dfd)
      >>> ncf_special = special.ncfdtr(dfn, dfd, 0, x)
  
      >>> fig = plt.figure()
      >>> ax = fig.add_subplot(111)
      >>> ax.plot(x, ncf_stats, 'b-', lw=3)
      >>> ax.plot(x, ncf_special, 'r-')
      >>> plt.show()
  
      """)
  
  add_newdoc("scipy.special", "ncfdtri",
      """
      ncfdtri(p, dfn, dfd, nc)
  
      Inverse cumulative distribution function of the non-central F distribution.
  
      See `ncfdtr` for more details.
  
      """)
  
  add_newdoc("scipy.special", "ncfdtridfd",
      """
      ncfdtridfd(p, f, dfn, nc)
  
      Calculate degrees of freedom (denominator) for the noncentral F-distribution.
  
      See `ncfdtr` for more details.
  
      Notes
      -----
      The value of the cumulative noncentral F distribution is not necessarily
      monotone in either degrees of freedom.  There thus may be two values that
      provide a given CDF value.  This routine assumes monotonicity and will
      find an arbitrary one of the two values.
  
      """)
  
  add_newdoc("scipy.special", "ncfdtridfn",
      """
      ncfdtridfn(p, f, dfd, nc)
  
      Calculate degrees of freedom (numerator) for the noncentral F-distribution.
  
      See `ncfdtr` for more details.
  
      Notes
      -----
      The value of the cumulative noncentral F distribution is not necessarily
      monotone in either degrees of freedom.  There thus may be two values that
      provide a given CDF value.  This routine assumes monotonicity and will
      find an arbitrary one of the two values.
  
      """)
  
  add_newdoc("scipy.special", "ncfdtrinc",
      """
      ncfdtrinc(p, f, dfn, dfd)
  
      Calculate non-centrality parameter for non-central F distribution.
  
      See `ncfdtr` for more details.
  
      """)
  
  add_newdoc("scipy.special", "nctdtr",
      """
      nctdtr(df, nc, t)
  
      Cumulative distribution function of the non-central `t` distribution.
  
      Parameters
      ----------
      df : array_like
          Degrees of freedom of the distribution.  Should be in range (0, inf).
      nc : array_like
          Noncentrality parameter.  Should be in range (-1e6, 1e6).
      t : array_like
          Quantiles, i.e. the upper limit of integration.
  
      Returns
      -------
      cdf : float or ndarray
          The calculated CDF.  If all inputs are scalar, the return will be a
          float.  Otherwise it will be an array.
  
      See Also
      --------
      nctdtrit : Inverse CDF (iCDF) of the non-central t distribution.
      nctdtridf : Calculate degrees of freedom, given CDF and iCDF values.
      nctdtrinc : Calculate non-centrality parameter, given CDF iCDF values.
  
      Examples
      --------
      >>> from scipy import special
      >>> from scipy import stats
      >>> import matplotlib.pyplot as plt
  
      Plot the CDF of the non-central t distribution, for nc=0.  Compare with the
      t-distribution from scipy.stats:
  
      >>> x = np.linspace(-5, 5, num=500)
      >>> df = 3
      >>> nct_stats = stats.t.cdf(x, df)
      >>> nct_special = special.nctdtr(df, 0, x)
  
      >>> fig = plt.figure()
      >>> ax = fig.add_subplot(111)
      >>> ax.plot(x, nct_stats, 'b-', lw=3)
      >>> ax.plot(x, nct_special, 'r-')
      >>> plt.show()
  
      """)
  
  add_newdoc("scipy.special", "nctdtridf",
      """
      nctdtridf(p, nc, t)
  
      Calculate degrees of freedom for non-central t distribution.
  
      See `nctdtr` for more details.
  
      Parameters
      ----------
      p : array_like
          CDF values, in range (0, 1].
      nc : array_like
          Noncentrality parameter.  Should be in range (-1e6, 1e6).
      t : array_like
          Quantiles, i.e. the upper limit of integration.
  
      """)
  
  add_newdoc("scipy.special", "nctdtrinc",
      """
      nctdtrinc(df, p, t)
  
      Calculate non-centrality parameter for non-central t distribution.
  
      See `nctdtr` for more details.
  
      Parameters
      ----------
      df : array_like
          Degrees of freedom of the distribution.  Should be in range (0, inf).
      p : array_like
          CDF values, in range (0, 1].
      t : array_like
          Quantiles, i.e. the upper limit of integration.
  
      """)
  
  add_newdoc("scipy.special", "nctdtrit",
      """
      nctdtrit(df, nc, p)
  
      Inverse cumulative distribution function of the non-central t distribution.
  
      See `nctdtr` for more details.
  
      Parameters
      ----------
      df : array_like
          Degrees of freedom of the distribution.  Should be in range (0, inf).
      nc : array_like
          Noncentrality parameter.  Should be in range (-1e6, 1e6).
      p : array_like
          CDF values, in range (0, 1].
  
      """)
  
  add_newdoc("scipy.special", "ndtr",
      r"""
      ndtr(x)
  
      Gaussian cumulative distribution function.
  
      Returns the area under the standard Gaussian probability
      density function, integrated from minus infinity to `x`
  
      .. math::
  
         \frac{1}{\sqrt{2\pi}} \int_{-\infty}^x \exp(-t^2/2) dt
  
      Parameters
      ----------
      x : array_like, real or complex
          Argument
  
      Returns
      -------
      ndarray
          The value of the normal CDF evaluated at `x`
  
      See Also
      --------
      erf
      erfc
      scipy.stats.norm
      log_ndtr
  
      """)
  
  
  add_newdoc("scipy.special", "nrdtrimn",
      """
      nrdtrimn(p, x, std)
  
      Calculate mean of normal distribution given other params.
  
      Parameters
      ----------
      p : array_like
          CDF values, in range (0, 1].
      x : array_like
          Quantiles, i.e. the upper limit of integration.
      std : array_like
          Standard deviation.
  
      Returns
      -------
      mn : float or ndarray
          The mean of the normal distribution.
  
      See Also
      --------
      nrdtrimn, ndtr
  
      """)
  
  add_newdoc("scipy.special", "nrdtrisd",
      """
      nrdtrisd(p, x, mn)
  
      Calculate standard deviation of normal distribution given other params.
  
      Parameters
      ----------
      p : array_like
          CDF values, in range (0, 1].
      x : array_like
          Quantiles, i.e. the upper limit of integration.
      mn : float or ndarray
          The mean of the normal distribution.
  
      Returns
      -------
      std : array_like
          Standard deviation.
  
      See Also
      --------
      nrdtristd, ndtr
  
      """)
  
  add_newdoc("scipy.special", "log_ndtr",
      """
      log_ndtr(x)
  
      Logarithm of Gaussian cumulative distribution function.
  
      Returns the log of the area under the standard Gaussian probability
      density function, integrated from minus infinity to `x`::
  
          log(1/sqrt(2*pi) * integral(exp(-t**2 / 2), t=-inf..x))
  
      Parameters
      ----------
      x : array_like, real or complex
          Argument
  
      Returns
      -------
      ndarray
          The value of the log of the normal CDF evaluated at `x`
  
      See Also
      --------
      erf
      erfc
      scipy.stats.norm
      ndtr
  
      """)
  
  add_newdoc("scipy.special", "ndtri",
      """
      ndtri(y)
  
      Inverse of `ndtr` vs x
  
      Returns the argument x for which the area under the Gaussian
      probability density function (integrated from minus infinity to `x`)
      is equal to y.
      """)
  
  add_newdoc("scipy.special", "obl_ang1",
      """
      obl_ang1(m, n, c, x)
  
      Oblate spheroidal angular function of the first kind and its derivative
  
      Computes the oblate spheroidal angular function of the first kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "obl_ang1_cv",
      """
      obl_ang1_cv(m, n, c, cv, x)
  
      Oblate spheroidal angular function obl_ang1 for precomputed characteristic value
  
      Computes the oblate spheroidal angular function of the first kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``. Requires
      pre-computed characteristic value.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "obl_cv",
      """
      obl_cv(m, n, c)
  
      Characteristic value of oblate spheroidal function
  
      Computes the characteristic value of oblate spheroidal wave
      functions of order `m`, `n` (n>=m) and spheroidal parameter `c`.
      """)
  
  add_newdoc("scipy.special", "obl_rad1",
      """
      obl_rad1(m, n, c, x)
  
      Oblate spheroidal radial function of the first kind and its derivative
  
      Computes the oblate spheroidal radial function of the first kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "obl_rad1_cv",
      """
      obl_rad1_cv(m, n, c, cv, x)
  
      Oblate spheroidal radial function obl_rad1 for precomputed characteristic value
  
      Computes the oblate spheroidal radial function of the first kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``. Requires
      pre-computed characteristic value.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "obl_rad2",
      """
      obl_rad2(m, n, c, x)
  
      Oblate spheroidal radial function of the second kind and its derivative.
  
      Computes the oblate spheroidal radial function of the second kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "obl_rad2_cv",
      """
      obl_rad2_cv(m, n, c, cv, x)
  
      Oblate spheroidal radial function obl_rad2 for precomputed characteristic value
  
      Computes the oblate spheroidal radial function of the second kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``. Requires
      pre-computed characteristic value.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pbdv",
      """
      pbdv(v, x)
  
      Parabolic cylinder function D
  
      Returns (d, dp) the parabolic cylinder function Dv(x) in d and the
      derivative, Dv'(x) in dp.
  
      Returns
      -------
      d
          Value of the function
      dp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pbvv",
      """
      pbvv(v, x)
  
      Parabolic cylinder function V
  
      Returns the parabolic cylinder function Vv(x) in v and the
      derivative, Vv'(x) in vp.
  
      Returns
      -------
      v
          Value of the function
      vp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pbwa",
      """
      pbwa(a, x)
  
      Parabolic cylinder function W
  
      Returns the parabolic cylinder function W(a, x) in w and the
      derivative, W'(a, x) in wp.
  
      .. warning::
  
         May not be accurate for large (>5) arguments in a and/or x.
  
      Returns
      -------
      w
          Value of the function
      wp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pdtr",
      """
      pdtr(k, m)
  
      Poisson cumulative distribution function
  
      Returns the sum of the first `k` terms of the Poisson distribution:
      sum(exp(-m) * m**j / j!, j=0..k) = gammaincc( k+1, m).  Arguments
      must both be positive and `k` an integer.
      """)
  
  add_newdoc("scipy.special", "pdtrc",
      """
      pdtrc(k, m)
  
      Poisson survival function
  
      Returns the sum of the terms from k+1 to infinity of the Poisson
      distribution: sum(exp(-m) * m**j / j!, j=k+1..inf) = gammainc(
      k+1, m).  Arguments must both be positive and `k` an integer.
      """)
  
  add_newdoc("scipy.special", "pdtri",
      """
      pdtri(k, y)
  
      Inverse to `pdtr` vs m
  
      Returns the Poisson variable `m` such that the sum from 0 to `k` of
      the Poisson density is equal to the given probability `y`:
      calculated by gammaincinv(k+1, y). `k` must be a nonnegative
      integer and `y` between 0 and 1.
      """)
  
  add_newdoc("scipy.special", "pdtrik",
      """
      pdtrik(p, m)
  
      Inverse to `pdtr` vs k
  
      Returns the quantile k such that ``pdtr(k, m) = p``
      """)
  
  add_newdoc("scipy.special", "poch",
      """
      poch(z, m)
  
      Rising factorial (z)_m
  
      The Pochhammer symbol (rising factorial), is defined as::
  
          (z)_m = gamma(z + m) / gamma(z)
  
      For positive integer `m` it reads::
  
          (z)_m = z * (z + 1) * ... * (z + m - 1)
      """)
  
  add_newdoc("scipy.special", "pro_ang1",
      """
      pro_ang1(m, n, c, x)
  
      Prolate spheroidal angular function of the first kind and its derivative
  
      Computes the prolate spheroidal angular function of the first kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pro_ang1_cv",
      """
      pro_ang1_cv(m, n, c, cv, x)
  
      Prolate spheroidal angular function pro_ang1 for precomputed characteristic value
  
      Computes the prolate spheroidal angular function of the first kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``. Requires
      pre-computed characteristic value.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pro_cv",
      """
      pro_cv(m, n, c)
  
      Characteristic value of prolate spheroidal function
  
      Computes the characteristic value of prolate spheroidal wave
      functions of order `m`, `n` (n>=m) and spheroidal parameter `c`.
      """)
  
  add_newdoc("scipy.special", "pro_rad1",
      """
      pro_rad1(m, n, c, x)
  
      Prolate spheroidal radial function of the first kind and its derivative
  
      Computes the prolate spheroidal radial function of the first kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pro_rad1_cv",
      """
      pro_rad1_cv(m, n, c, cv, x)
  
      Prolate spheroidal radial function pro_rad1 for precomputed characteristic value
  
      Computes the prolate spheroidal radial function of the first kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``. Requires
      pre-computed characteristic value.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pro_rad2",
      """
      pro_rad2(m, n, c, x)
  
      Prolate spheroidal radial function of the secon kind and its derivative
  
      Computes the prolate spheroidal radial function of the second kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pro_rad2_cv",
      """
      pro_rad2_cv(m, n, c, cv, x)
  
      Prolate spheroidal radial function pro_rad2 for precomputed characteristic value
  
      Computes the prolate spheroidal radial function of the second kind
      and its derivative (with respect to `x`) for mode parameters m>=0
      and n>=m, spheroidal parameter `c` and ``|x| < 1.0``. Requires
      pre-computed characteristic value.
  
      Returns
      -------
      s
          Value of the function
      sp
          Value of the derivative vs x
      """)
  
  add_newdoc("scipy.special", "pseudo_huber",
      r"""
      pseudo_huber(delta, r)
  
      Pseudo-Huber loss function.
  
      .. math:: \mathrm{pseudo\_huber}(\delta, r) = \delta^2 \left( \sqrt{ 1 + \left( \frac{r}{\delta} \right)^2 } - 1 \right)
  
      Parameters
      ----------
      delta : ndarray
          Input array, indicating the soft quadratic vs. linear loss changepoint.
      r : ndarray
          Input array, possibly representing residuals.
  
      Returns
      -------
      res : ndarray
          The computed Pseudo-Huber loss function values.
  
      Notes
      -----
      This function is convex in :math:`r`.
  
      .. versionadded:: 0.15.0
  
      """)
  
  add_newdoc("scipy.special", "psi",
      """
      psi(z, out=None)
  
      The digamma function.
  
      The logarithmic derivative of the gamma function evaluated at ``z``.
  
      Parameters
      ----------
      z : array_like
          Real or complex argument.
      out : ndarray, optional
          Array for the computed values of ``psi``.
  
      Returns
      -------
      digamma : ndarray
          Computed values of ``psi``.
  
      Notes
      -----
      For large values not close to the negative real axis ``psi`` is
      computed using the asymptotic series (5.11.2) from [1]_. For small
      arguments not close to the negative real axis the recurrence
      relation (5.5.2) from [1]_ is used until the argument is large
      enough to use the asymptotic series. For values close to the
      negative real axis the reflection formula (5.5.4) from [1]_ is
      used first.  Note that ``psi`` has a family of zeros on the
      negative real axis which occur between the poles at nonpositive
      integers. Around the zeros the reflection formula suffers from
      cancellation and the implementation loses precision. The sole
      positive zero and the first negative zero, however, are handled
      separately by precomputing series expansions using [2]_, so the
      function should maintain full accuracy around the origin.
  
      References
      ----------
      .. [1] NIST Digital Library of Mathematical Functions
             http://dlmf.nist.gov/5
      .. [2] Fredrik Johansson and others.
             "mpmath: a Python library for arbitrary-precision floating-point arithmetic"
             (Version 0.19) http://mpmath.org/
  
      """)
  
  add_newdoc("scipy.special", "radian",
      """
      radian(d, m, s)
  
      Convert from degrees to radians
  
      Returns the angle given in (d)egrees, (m)inutes, and (s)econds in
      radians.
      """)
  
  add_newdoc("scipy.special", "rel_entr",
      r"""
      rel_entr(x, y)
  
      Elementwise function for computing relative entropy.
  
      .. math:: \mathrm{rel\_entr}(x, y) = \begin{cases} x \log(x / y) & x > 0, y > 0 \\ 0 & x = 0, y \ge 0 \\ \infty & \text{otherwise} \end{cases}
  
      Parameters
      ----------
      x : ndarray
          First input array.
      y : ndarray
          Second input array.
  
      Returns
      -------
      res : ndarray
          Output array.
  
      See Also
      --------
      entr, kl_div
  
      Notes
      -----
      This function is jointly convex in x and y.
  
      .. versionadded:: 0.15.0
  
      """)
  
  add_newdoc("scipy.special", "rgamma",
      """
      rgamma(z)
  
      Gamma function inverted
  
      Returns ``1/gamma(x)``
      """)
  
  add_newdoc("scipy.special", "round",
      """
      round(x)
  
      Round to nearest integer
  
      Returns the nearest integer to `x` as a double precision floating
      point result.  If `x` ends in 0.5 exactly, the nearest even integer
      is chosen.
      """)
  
  add_newdoc("scipy.special", "shichi",
      r"""
      shichi(x, out=None)
  
      Hyperbolic sine and cosine integrals.
  
      The hyperbolic sine integral is
  
      .. math::
  
        \int_0^x \frac{\sinh{t}}{t}dt
  
      and the hyperbolic cosine integral is
  
      .. math::
  
        \gamma + \log(x) + \int_0^x \frac{\cosh{t} - 1}{t} dt
  
      where :math:`\gamma` is Euler's constant and :math:`\log` is the
      principle branch of the logarithm.
  
      Parameters
      ----------
      x : array_like
          Real or complex points at which to compute the hyperbolic sine
          and cosine integrals.
  
      Returns
      -------
      si : ndarray
          Hyperbolic sine integral at ``x``
      ci : ndarray
          Hyperbolic cosine integral at ``x``
  
      Notes
      -----
      For real arguments with ``x < 0``, ``chi`` is the real part of the
      hyperbolic cosine integral. For such points ``chi(x)`` and ``chi(x
      + 0j)`` differ by a factor of ``1j*pi``.
  
      For real arguments the function is computed by calling Cephes'
      [1]_ *shichi* routine. For complex arguments the algorithm is based
      on Mpmath's [2]_ *shi* and *chi* routines.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      .. [2] Fredrik Johansson and others.
             "mpmath: a Python library for arbitrary-precision floating-point arithmetic"
             (Version 0.19) http://mpmath.org/
      """)
  
  add_newdoc("scipy.special", "sici",
      r"""
      sici(x, out=None)
  
      Sine and cosine integrals.
  
      The sine integral is
  
      .. math::
      
        \int_0^x \frac{\sin{t}}{t}dt
  
      and the cosine integral is
  
      .. math::
  
        \gamma + \log(x) + \int_0^x \frac{\cos{t} - 1}{t}dt
  
      where :math:`\gamma` is Euler's constant and :math:`\log` is the
      principle branch of the logarithm.
  
      Parameters
      ----------
      x : array_like
          Real or complex points at which to compute the sine and cosine
          integrals.
  
      Returns
      -------
      si : ndarray
          Sine integral at ``x``
      ci : ndarray
          Cosine integral at ``x``
  
      Notes
      -----
      For real arguments with ``x < 0``, ``ci`` is the real part of the
      cosine integral. For such points ``ci(x)`` and ``ci(x + 0j)``
      differ by a factor of ``1j*pi``.
  
      For real arguments the function is computed by calling Cephes'
      [1]_ *sici* routine. For complex arguments the algorithm is based
      on Mpmath's [2]_ *si* and *ci* routines.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      .. [2] Fredrik Johansson and others.
             "mpmath: a Python library for arbitrary-precision floating-point arithmetic"
             (Version 0.19) http://mpmath.org/
      """)
  
  add_newdoc("scipy.special", "sindg",
      """
      sindg(x)
  
      Sine of angle given in degrees
      """)
  
  add_newdoc("scipy.special", "smirnov",
      """
      smirnov(n, e)
  
      Kolmogorov-Smirnov complementary cumulative distribution function
  
      Returns the exact Kolmogorov-Smirnov complementary cumulative
      distribution function (Dn+ or Dn-) for a one-sided test of
      equality between an empirical and a theoretical distribution. It
      is equal to the probability that the maximum difference between a
      theoretical distribution and an empirical one based on `n` samples
      is greater than e.
      """)
  
  add_newdoc("scipy.special", "smirnovi",
      """
      smirnovi(n, y)
  
      Inverse to `smirnov`
  
      Returns ``e`` such that ``smirnov(n, e) = y``.
      """)
  
  add_newdoc("scipy.special", "spence",
      r"""
      spence(z)
  
      Spence's function, also known as the dilogarithm. It is defined to
      be
  
      .. math::
        \int_0^z \frac{\log(t)}{1 - t}dt
  
      for complex :math:`z`, where the contour of integration is taken
      to avoid the branch cut of the logarithm. Spence's function is
      analytic everywhere except the negative real axis where it has a
      branch cut.
  
      Note that there is a different convention which defines Spence's
      function by the integral
  
      .. math::
        -\int_0^z \frac{\log(1 - t)}{t}dt;
  
      this is our ``spence(1 - z)``.
  
      """)
  
  add_newdoc("scipy.special", "stdtr",
      """
      stdtr(df, t)
  
      Student t distribution cumulative density function
  
      Returns the integral from minus infinity to t of the Student t
      distribution with df > 0 degrees of freedom::
  
         gamma((df+1)/2)/(sqrt(df*pi)*gamma(df/2)) *
         integral((1+x**2/df)**(-df/2-1/2), x=-inf..t)
  
      """)
  
  add_newdoc("scipy.special", "stdtridf",
      """
      stdtridf(p, t)
  
      Inverse of `stdtr` vs df
  
      Returns the argument df such that stdtr(df, t) is equal to `p`.
      """)
  
  add_newdoc("scipy.special", "stdtrit",
      """
      stdtrit(df, p)
  
      Inverse of `stdtr` vs `t`
  
      Returns the argument `t` such that stdtr(df, t) is equal to `p`.
      """)
  
  add_newdoc("scipy.special", "struve",
      r"""
      struve(v, x)
  
      Struve function.
  
      Return the value of the Struve function of order `v` at `x`.  The Struve
      function is defined as,
  
      .. math::
          H_v(x) = (z/2)^{v + 1} \sum_{n=0}^\infty \frac{(-1)^n (z/2)^{2n}}{\Gamma(n + \frac{3}{2}) \Gamma(n + v + \frac{3}{2})},
  
      where :math:`\Gamma` is the gamma function.
  
      Parameters
      ----------
      v : array_like
          Order of the Struve function (float).
      x : array_like
          Argument of the Struve function (float; must be positive unless `v` is
          an integer).
  
      Returns
      -------
      H : ndarray
          Value of the Struve function of order `v` at `x`.
  
      Notes
      -----
      Three methods discussed in [1]_ are used to evaluate the Struve function:
  
      - power series
      - expansion in Bessel functions (if :math:`|z| < |v| + 20`)
      - asymptotic large-z expansion (if :math:`z \geq 0.7v + 12`)
  
      Rounding errors are estimated based on the largest terms in the sums, and
      the result associated with the smallest error is returned.
  
      See also
      --------
      modstruve
  
      References
      ----------
      .. [1] NIST Digital Library of Mathematical Functions
             http://dlmf.nist.gov/11
  
      """)
  
  add_newdoc("scipy.special", "tandg",
      """
      tandg(x)
  
      Tangent of angle x given in degrees.
      """)
  
  add_newdoc("scipy.special", "tklmbda",
      """
      tklmbda(x, lmbda)
  
      Tukey-Lambda cumulative distribution function
  
      """)
  
  add_newdoc("scipy.special", "wofz",
      """
      wofz(z)
  
      Faddeeva function
  
      Returns the value of the Faddeeva function for complex argument::
  
          exp(-z**2) * erfc(-i*z)
  
      See Also
      --------
      dawsn, erf, erfc, erfcx, erfi
  
      References
      ----------
      .. [1] Steven G. Johnson, Faddeeva W function implementation.
         http://ab-initio.mit.edu/Faddeeva
  
      Examples
      --------
      >>> from scipy import special
      >>> import matplotlib.pyplot as plt
      >>> x = np.linspace(-3, 3)
      >>> plt.plot(x, special.wofz(x))
      >>> plt.xlabel('$x$')
      >>> plt.ylabel('$wofz(x)$')
      >>> plt.show()
  
      """)
  
  add_newdoc("scipy.special", "xlogy",
      """
      xlogy(x, y)
  
      Compute ``x*log(y)`` so that the result is 0 if ``x = 0``.
  
      Parameters
      ----------
      x : array_like
          Multiplier
      y : array_like
          Argument
  
      Returns
      -------
      z : array_like
          Computed x*log(y)
  
      Notes
      -----
  
      .. versionadded:: 0.13.0
  
      """)
  
  add_newdoc("scipy.special", "xlog1py",
      """
      xlog1py(x, y)
  
      Compute ``x*log1p(y)`` so that the result is 0 if ``x = 0``.
  
      Parameters
      ----------
      x : array_like
          Multiplier
      y : array_like
          Argument
  
      Returns
      -------
      z : array_like
          Computed x*log1p(y)
  
      Notes
      -----
  
      .. versionadded:: 0.13.0
  
      """)
  
  add_newdoc("scipy.special", "y0",
      r"""
      y0(x)
  
      Bessel function of the second kind of order 0.
  
      Parameters
      ----------
      x : array_like
          Argument (float).
  
      Returns
      -------
      Y : ndarray
          Value of the Bessel function of the second kind of order 0 at `x`.
  
      Notes
      -----
      
      The domain is divided into the intervals [0, 5] and (5, infinity). In the
      first interval a rational approximation :math:`R(x)` is employed to
      compute,
      
      .. math::
          
          Y_0(x) = R(x) + \frac{2 \log(x) J_0(x)}{\pi},
  
      where :math:`J_0` is the Bessel function of the first kind of order 0.
  
      In the second interval, the Hankel asymptotic expansion is employed with
      two rational functions of degree 6/6 and 7/7.
  
      This function is a wrapper for the Cephes [1]_ routine `y0`.
  
      See also
      --------
      j0
      yv
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "y1",
      """
      y1(x)
  
      Bessel function of the second kind of order 1.
  
      Parameters
      ----------
      x : array_like
          Argument (float).
  
      Returns
      -------
      Y : ndarray
          Value of the Bessel function of the second kind of order 1 at `x`.
  
      Notes
      -----
  
      The domain is divided into the intervals [0, 8] and (8, infinity). In the
      first interval a 25 term Chebyshev expansion is used, and computing
      :math:`J_1` (the Bessel function of the first kind) is required. In the
      second, the asymptotic trigonometric representation is employed using two
      rational functions of degree 5/5.
  
      This function is a wrapper for the Cephes [1]_ routine `y1`.
  
      See also
      --------
      j1
      yn
      yv
      
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "yn",
      r"""
      yn(n, x)
  
      Bessel function of the second kind of integer order and real argument.
  
      Parameters
      ----------
      n : array_like
          Order (integer).
      z : array_like
          Argument (float).
  
      Returns
      -------
      Y : ndarray
          Value of the Bessel function, :math:`Y_n(x)`.
  
      Notes
      -----
      Wrapper for the Cephes [1]_ routine `yn`.
  
      The function is evaluated by forward recurrence on `n`, starting with
      values computed by the Cephes routines `y0` and `y1`. If `n = 0` or 1,
      the routine for `y0` or `y1` is called directly.
  
      See also
      --------
      yv : For real order and real or complex argument.
  
      References
      ----------
      .. [1] Cephes Mathematical Functions Library,
             http://www.netlib.org/cephes/index.html
      """)
  
  add_newdoc("scipy.special", "yv",
      r"""
      yv(v, z)
  
      Bessel function of the second kind of real order and complex argument.
  
      Parameters
      ----------
      v : array_like
          Order (float).
      z : array_like
          Argument (float or complex).
  
      Returns
      -------
      Y : ndarray
          Value of the Bessel function of the second kind, :math:`Y_v(x)`.
  
      Notes
      -----
      For positive `v` values, the computation is carried out using the
      AMOS [1]_ `zbesy` routine, which exploits the connection to the Hankel
      Bessel functions :math:`H_v^{(1)}` and :math:`H_v^{(2)}`,
  
      .. math:: Y_v(z) = \frac{1}{2\imath} (H_v^{(1)} - H_v^{(2)}).
  
      For negative `v` values the formula,
  
      .. math:: Y_{-v}(z) = Y_v(z) \cos(\pi v) + J_v(z) \sin(\pi v)
  
      is used, where :math:`J_v(z)` is the Bessel function of the first kind,
      computed using the AMOS routine `zbesj`.  Note that the second term is
      exactly zero for integer `v`; to improve accuracy the second term is
      explicitly omitted for `v` values such that `v = floor(v)`.
  
      See also
      --------
      yve : :math:`Y_v` with leading exponential behavior stripped off.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
  
      """)
  
  add_newdoc("scipy.special", "yve",
      r"""
      yve(v, z)
  
      Exponentially scaled Bessel function of the second kind of real order.
  
      Returns the exponentially scaled Bessel function of the second
      kind of real order `v` at complex `z`::
  
          yve(v, z) = yv(v, z) * exp(-abs(z.imag))
  
      Parameters
      ----------
      v : array_like
          Order (float).
      z : array_like
          Argument (float or complex).
  
      Returns
      -------
      Y : ndarray
          Value of the exponentially scaled Bessel function.
  
      Notes
      -----
      For positive `v` values, the computation is carried out using the
      AMOS [1]_ `zbesy` routine, which exploits the connection to the Hankel
      Bessel functions :math:`H_v^{(1)}` and :math:`H_v^{(2)}`,
  
      .. math:: Y_v(z) = \frac{1}{2\imath} (H_v^{(1)} - H_v^{(2)}).
  
      For negative `v` values the formula,
  
      .. math:: Y_{-v}(z) = Y_v(z) \cos(\pi v) + J_v(z) \sin(\pi v)
  
      is used, where :math:`J_v(z)` is the Bessel function of the first kind,
      computed using the AMOS routine `zbesj`.  Note that the second term is
      exactly zero for integer `v`; to improve accuracy the second term is
      explicitly omitted for `v` values such that `v = floor(v)`.
  
      References
      ----------
      .. [1] Donald E. Amos, "AMOS, A Portable Package for Bessel Functions
             of a Complex Argument and Nonnegative Order",
             http://netlib.org/amos/
      """)
  
  add_newdoc("scipy.special", "_zeta",
      """
      _zeta(x, q)
  
      Internal function, Hurwitz zeta.
  
      """)
  
  add_newdoc("scipy.special", "zetac",
      """
      zetac(x)
  
      Riemann zeta function minus 1.
  
      This function is defined as
  
      .. math:: \\zeta(x) = \\sum_{k=2}^{\\infty} 1 / k^x,
  
      where ``x > 1``.
  
      See Also
      --------
      zeta
  
      """)
  
  add_newdoc("scipy.special", "_struve_asymp_large_z",
      """
      _struve_asymp_large_z(v, z, is_h)
  
      Internal function for testing `struve` & `modstruve`
  
      Evaluates using asymptotic expansion
  
      Returns
      -------
      v, err
      """)
  
  add_newdoc("scipy.special", "_struve_power_series",
      """
      _struve_power_series(v, z, is_h)
  
      Internal function for testing `struve` & `modstruve`
  
      Evaluates using power series
  
      Returns
      -------
      v, err
      """)
  
  add_newdoc("scipy.special", "_struve_bessel_series",
      """
      _struve_bessel_series(v, z, is_h)
  
      Internal function for testing `struve` & `modstruve`
  
      Evaluates using Bessel function series
  
      Returns
      -------
      v, err
      """)
  
  add_newdoc("scipy.special", "_spherical_jn",
      """
      Internal function, use `spherical_jn` instead.
      """)
  
  add_newdoc("scipy.special", "_spherical_jn_d",
      """
      Internal function, use `spherical_jn` instead.
      """)
  
  add_newdoc("scipy.special", "_spherical_yn",
      """
      Internal function, use `spherical_yn` instead.
      """)
  
  add_newdoc("scipy.special", "_spherical_yn_d",
      """
      Internal function, use `spherical_yn` instead.
      """)
  
  add_newdoc("scipy.special", "_spherical_in",
      """
      Internal function, use `spherical_in` instead.
      """)
  
  add_newdoc("scipy.special", "_spherical_in_d",
      """
      Internal function, use `spherical_in` instead.
      """)
  
  add_newdoc("scipy.special", "_spherical_kn",
      """
      Internal function, use `spherical_kn` instead.
      """)
  
  add_newdoc("scipy.special", "_spherical_kn_d",
      """
      Internal function, use `spherical_kn` instead.
      """)
  
  add_newdoc("scipy.special", "loggamma",
      r"""
      loggamma(z, out=None)
  
      Principal branch of the logarithm of the Gamma function. It is
      defined to be :math:`\log(\Gamma(x))` for :math:`x > 0` and
      extended to the complex plane by analytic continuation. The
      implementation here is based on [hare1997]_.
  
      The function has a single branch cut on the negative real axis and
      is taken to be continuous when approaching the axis from
      above. Note that it is not generally true that
      :math:`\log\Gamma(z) = \log(\Gamma(z))`, though the real parts of
      the functions do agree. The benefit of not defining ``loggamma``
      as :math:`\log(\Gamma(z))` is that the latter function has a
      complicated branch cut structure whereas ``loggamma`` is analytic
      except for on the negative real axis.
  
      The identities
  
      .. math::
        \exp(\log\Gamma(z)) &= \Gamma(z) \\
        \log\Gamma(z + 1) &= \log(z) + \log\Gamma(z)
  
      make ``loggama`` useful for working in complex logspace. However,
      ``loggamma`` necessarily returns complex outputs for real inputs,
      so if you want to work only with real numbers use `gammaln`. On
      the real line the two functions are related by ``exp(loggamma(x))
      = gammasgn(x)*exp(gammaln(x))``, though in practice rounding
      errors will introduce small spurious imaginary components in
      ``exp(loggamma(x))``.
  
      .. versionadded:: 0.18.0
  
      Parameters
      ----------
      z : array-like
          Values in the complex plain at which to compute ``loggamma``
      out : ndarray, optional
          Output array for computed values of ``loggamma``
  
      Returns
      -------
      loggamma : ndarray
          Values of ``loggamma`` at z.
  
      See also
      --------
      gammaln : logarithm of the absolute value of the Gamma function
      gammasgn : sign of the gamma function
  
      References
      ----------
      .. [hare1997] D.E.G. Hare,
        *Computing the Principal Branch of log-Gamma*,
        Journal of Algorithms, Volume 25, Issue 2, November 1997, pages 221-236.
      """)
  
  add_newdoc("scipy.special", "_sinpi",
      """
      Internal function, do not use.
      """)
  
  add_newdoc("scipy.special", "_cospi",
      """
      Internal function, do not use.
      """)
  